The galaxy appears as a centrally concentrated elliptical object, exhibiting a smooth, almost featureless morphology. The core is characterized by a bright, yellowish-white hue, suggestive of an older stellar population. The color gradually shifts towards a redder tone in the outer regions. The radial intensity profile decreases smoothly outward, indicating a lack of significant substructure or prominent spiral arms. The overall shape appears generally round, with a minor ellipticity. There is no obvious evidence of ongoing mergers or tidal disturbances, although subtle asymmetries may be present.
