The galaxy appears to be a relatively smooth, centrally concentrated object. The light distribution suggests it is an elliptical galaxy, or potentially a spiral galaxy seen face-on with a dominant bulge. There is some indication of a slight elongation, though the galaxy is mostly round. Faint hints of diffuse, extended light are present, suggesting a stellar halo surrounding the main body. There is little evidence of distinct spiral arm structure or prominent dust lanes. The galaxy exhibits a color profile suggesting an older stellar population, with a somewhat redder hue. A slight asymmetry in the outer regions could indicate a minor gravitational interaction or recent accretion event, though the galaxy’s overall morphology appears relatively undisturbed.
