The galaxy presents as an elongated structure, viewed nearly edge-on. A prominent central bulge, exhibiting a yellowish hue, dominates the galaxy's core, with a color gradient suggesting an older stellar population. The disk appears thin and is oriented almost horizontally in the image. There is evidence of dust lanes or obscuring material along the galactic plane, particularly visible as subtle dark regions embedded within the fainter disk. The disk itself exhibits a smoother texture, suggesting that it might be composed of less star formation. Based on the apparent lack of strong blue emission, a relatively low star formation rate is inferred, as well as a very high mass and low specific star formation rate. Faint indications of slight warping or tidal disturbances are suspected. This could indicate a prior or ongoing interaction, although no other merging activity is evident at this resolution. The apparent size and shape suggest it is a moderately large galaxy, and given the lack of spiral arm features, it seems to be either a lenticular or edge-on spiral galaxy with a suppressed rate of star formation. The bulge is likely more rounded in shape.
