The galaxy appears as a centrally concentrated object, with a smooth, spheroidal morphology dominating its overall structure. The core exhibits a yellowish-white hue, suggestive of an older stellar population. Fainter, bluish-white light extends outwards from the central region, indicating the presence of some younger stars and potentially ongoing star formation. This extended halo appears patchy, possibly indicating some disturbance within the galactic structure. There is a noticeable asymmetry in the outer regions, perhaps indicative of a past or ongoing minor merger event. A faint, reddish-orange patch is observable at the edge of the galaxy, indicating a small area of dust or a region of older stars.
