The galaxy presents as a generally smooth, centrally concentrated object. Its overall color profile suggests an older stellar population, with a dominant yellowish-orange hue indicative of evolved stars. There is a slight radial color gradient, with the central region appearing more intensely yellow-orange compared to the outer regions which fade into red.

The morphology appears largely spheroidal or elliptical. There is no readily apparent spiral arm structure or strong dust lane obscuration visible. The galaxy's light profile decreases smoothly outward from the core. There are no visually obvious signs of ongoing major merger activity or significant tidal disturbances. There may be some subtle irregularities in the outer isophotes, suggesting potentially minor interactions or past merger events, however, the resolution of the image limits conclusive assessment.
