The galaxy presents a generally smooth and elliptical morphology. The central region exhibits a concentrated, bright core, indicative of a significant stellar population and potentially a supermassive black hole at the galactic nucleus. The overall color profile suggests an evolved stellar population, leaning towards older, redder stars. There is a subtle color gradient moving outward from the core, with the outer regions exhibiting a slightly bluer hue suggesting the presence of some younger stars and perhaps a degree of ongoing, though limited, star formation. There is no clear evidence of spiral arm structure or a pronounced disk component; the light distribution is fairly uniform across the galaxy's body. Faint irregularities are seen in the galactic halo suggesting possible past mergers or tidal interactions.
