The galaxy presents a primarily smooth morphology, with a somewhat elliptical shape. The light distribution is concentrated towards the center, with a gradual decrease in intensity outward. The color gradient suggests an older stellar population. There is a small indication of a possible merging event, or at least some minor disturbance, given the asymmetry observed in the galaxy's outer regions. A substantial spheroidal component is indicated by the roundness of the galaxy's form. The overall color of the galaxy appears to be in the redder portion of the spectrum, possibly indicating a high mass. The lack of defined spiral arms or significant dust lanes supports its classification as a relatively passive system with a low star formation rate.
