The galaxy presents as a lenticular or possibly an edge-on spiral galaxy, characterized by a relatively smooth and elongated structure. It exhibits a central bulge that appears more condensed and brighter compared to the surrounding disc. The disc, although not clearly resolved into spiral arms, seems to have a flattened morphology. Overall, the light distribution within the galaxy is moderately smooth, with subtle variations in color and intensity across the structure. It appears that there may be a low rate of star formation. The galaxy is elongated, with a cigar-like appearance, suggesting a significant deviation from perfect circularity. There are no obvious signs of strong tidal distortions or interactions with other galaxies.
