The galaxy presents as a single, concentrated luminous region with a largely homogenous color profile. The color is predominantly yellowish, suggesting a stellar population that is primarily composed of older stars. There is no apparent spiral arm structure or distinct disk component visible. The morphology appears generally smooth and elliptical. Indications of any recent or ongoing star formation are minimal, inferred from the general lack of blue light. There is no strong indication of dust lanes, tidal tails, or other morphological features associated with mergers or significant gravitational disturbances. The overall appearance suggests a galaxy that is relatively evolved.
