The galaxy presents a smooth, rounded morphology, suggesting an elliptical classification. There is a concentrated central bulge with a bright, diffuse glow which transitions outwards to a fainter halo region. The lack of distinct spiral arms or a prominent disk indicates a relatively evolved system. The color profile appears to be a fairly uniform yellow-orange, possibly indicative of an older stellar population. The galaxy shows no signs of significant tidal disturbances or merging events. The overall structure suggests a relatively relaxed and dynamically stable system. Based on the galaxy's appearance, the star formation rate is likely low.
