The galaxy presents as a largely featureless elliptical or lenticular system. It exhibits a smooth, concentrated luminosity profile, with the highest intensity concentrated centrally. There is a gradual decrease in brightness moving outward from the core, suggesting a relatively old stellar population. The galaxy displays a generally spherical morphology. A subtle color gradient is noticeable, shifting from a more yellow-orange hue in the central regions to a slightly redder tone in the outskirts. This color shift is indicative of differences in stellar populations, where the central bulge may be dominated by older, metal-rich stars, and the outskirts may have comparatively younger, metal-poor stars. No spiral arm structure or dust lanes are visibly present. The overall appearance suggests a gravitationally relaxed, quiescent system, with little evidence of ongoing star formation.
