The galaxy presents as a yellowish, elliptical form with a concentrated central bulge. The light distribution appears relatively smooth and centrally concentrated, with a gradual decrease in intensity outwards from the core, which indicates an older stellar population. The galaxy displays a well-defined elliptical shape, exhibiting a moderate degree of ellipticity, with its light appearing fairly uniform. There seems to be a tidal interaction or minor disturbance on the outskirts of the main galactic body, implying a possible interaction or merger history, this is indicated by the less distinct glow on the right. The galaxy exhibits an evolved stellar population, indicative of a relatively low rate of star formation currently. The overall morphology indicates a fairly massive system.
