The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, appearing a yellow-white hue, indicative of an older stellar population. There are no obvious spiral arms or prominent dust lanes visible. The galaxy appears somewhat rounded in shape, with a slight elongation. There is little evidence of any major ongoing mergers or tidal disturbances. A diffuse, fainter halo surrounds the core, gradually fading into the background sky. The overall color suggests a moderate amount of recent or ongoing star formation activity.
