The galaxy presents as a diffuse, elliptical morphology with a smooth light profile, exhibiting a general lack of distinct spiral arm structures or prominent dust lanes. The central region displays a higher luminosity concentration, suggesting the presence of a galactic bulge. The overall color appears to be on the redder end of the spectrum, indicative of an older stellar population and potentially lower levels of ongoing star formation. There is a slight elongation in the galaxy's overall shape, deviating from a perfectly circular form, which might be a result of intrinsic morphology or a projection effect. A fainter, smaller companion galaxy is located close to the main galaxy which could be interacting or in the process of merging. However, there are no obvious signs of strong tidal disturbances or asymmetries. The lack of any apparent spiral structures and the smooth light profile could be suggestive of an early-type galaxy.
