The galaxy presents as a relatively smooth, elliptical morphology. The light is concentrated towards the center, suggesting a prominent galactic bulge. The lack of discernible spiral arms or distinct dust lanes indicates a featureless, rather homogenous structure. Its color index appears to be on the redder side, suggestive of an older stellar population with limited ongoing star formation. There is no visual evidence of any significant tidal disturbances or recent merger events; the overall symmetry supports a relaxed, undisturbed state. The galaxy shows a compact appearance with no clearly visible extended halo.
