The galaxy presents an overall smooth, elliptical morphology. The central region exhibits a high concentration of luminosity, appearing significantly brighter than the surrounding areas. This suggests a dense stellar population and potentially a supermassive black hole at its core.

There is a discernible color gradient. The central bulge displays a yellowish-red hue, indicating an older stellar population dominated by red giants. Moving outward from the core, the color becomes slightly bluer, hinting at the presence of younger, hotter stars, though their proportion appears relatively small.

While generally smooth, there is some faint mottling apparent in the outer regions. These subtle variations in surface brightness may indicate some low-level star formation activity or the presence of dust lanes. No distinct spiral arms or bar structures are visible. Overall, the galaxy appears relatively undisturbed, lacking any strong signs of recent merger events or tidal interactions. The overall appearance is consistent with an evolved, early-type galaxy.
