The galaxy appears to be a fairly luminous object, exhibiting a smooth, elliptical morphology. The light is concentrated towards the center, suggesting a large stellar bulge. The color profile is redder in the central region, possibly indicating an older stellar population or significant dust obscuration. Moving outward from the core, the galaxy transitions to a slightly bluer hue. This suggests the presence of a younger stellar population in the outer regions, possibly due to ongoing or recent star formation. Overall, the galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. The overall shape is somewhat elongated, indicating a moderate ellipticity.
