The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and rounded morphology. A bright, concentrated central bulge is apparent, indicating a high density of stars in the galactic nucleus. Moving outward from the core, a fainter, diffuse halo is observed. The color profile suggests an older stellar population, trending towards redder hues, but there is indication of some bluer, possibly younger, stars in the outer regions. No distinct spiral arms or prominent dust lanes are visible, supporting the classification as a relatively featureless system. The overall appearance suggests a galaxy that is not currently undergoing major interactions or mergers, though there is some slight irregularity in the outer edges, suggestive of minor past disturbances.
