The galaxy presents as a centrally concentrated, largely smooth elliptical structure with a slightly elongated morphology. Its core is a bright, concentrated region, surrounded by a fainter, more diffuse halo. Coloration appears to be predominantly yellowish-orange, suggesting a population of older stars. There is little evidence of spiral arms, dust lanes, or significant ongoing star formation within the visible light spectrum. The galaxy exhibits a general smoothness, indicating a lack of significant recent mergers or tidal disturbances, although there might be very faint hints of asymmetry in the outer halo. Overall, the galaxy appears to be a fairly evolved system.
