The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a generally round morphology, lacking any significant features such as spiral arms or a prominent disk structure. There are no readily apparent signs of ongoing major mergers or tidal disturbances, suggesting it is a relatively settled system. The galaxy displays a redder color profile, particularly towards the core, indicative of an older stellar population and potentially lower levels of active star formation within the galaxy. The overall luminosity is relatively high, suggesting a substantial stellar mass.
