The galaxy presents an elliptical morphology, appearing largely smooth and featureless. The light distribution indicates a centrally concentrated bulge that exhibits a gradual falloff in luminosity towards the outer regions. There is some faint indication of a possible disc structure, although it is not a prominent feature. The color is predominantly yellow-orange, indicating an older stellar population with a relatively low rate of ongoing star formation. There appears to be a secondary condensation of light to the side of the galaxy, but without further data, it's uncertain whether this is a tidal feature indicative of a recent interaction, a star forming region within the galaxy, or a background object. The galaxy is mostly symmetrical in appearance, and exhibits no clear signs of active merging or significant disruption. Overall, this galaxy appears to be a relatively evolved system with an intermediate mass.
