The galaxy presents as a somewhat luminous, moderately sized object with a generally elliptical morphology. The core region exhibits a concentrated, bright yellowish-white hue, indicative of an older stellar population and potentially a supermassive black hole. Moving outward from the core, the color gradually shifts to a slightly more diffuse yellowish-green, with very faint hints of blue, which suggests the presence of a younger, albeit subdued, stellar population in the outer regions. The overall structure appears relatively smooth with no obvious indications of spiral arms or significant dust lanes. There are no signs of major tidal disturbances or ongoing mergers, but there is a subtle asymmetry that could indicate minor disturbances. The galaxy's apparent roundness suggests that we are viewing it nearly face-on.
