This galaxy appears to be a relatively smooth, elliptical system. Its light profile is dominated by a central bulge, which exhibits a high degree of radial symmetry. There is little evidence of spiral arm structure or prominent dust lanes. The galaxy displays a slight elongation, suggesting a possible transition between an E0 and E3 morphological type. The color appears generally consistent across the galaxy, with a slightly redder hue overall, indicative of an older stellar population. There is a subtle suggestion of a faint, extended halo surrounding the main body of the galaxy, which could be indicative of past or ongoing minor merger activity.
