The galaxy appears as a relatively smooth, elliptical-shaped object. Its core presents a concentrated brightness, with a diffuse halo extending outward. The light distribution is not perfectly symmetrical; it seems slightly elongated along one axis, suggesting a possible deviation from a perfect spheroid. There's a subtle color gradient, appearing more yellow in the center and fading to redder hues towards the outer regions. This is likely indicative of an older stellar population in the central bulge compared to what is present at the galaxy's edge. The morphology appears largely undisturbed, with no obvious signs of active galactic nuclei, spiral arms, or major merger events. However, there may be a slight asymmetry suggesting a minor tidal disturbance or ongoing interaction. Its compact nature and relative lack of visible substructure suggest a low rate of star formation.
