The galaxy presents a generally smooth morphology, with no prominent spiral arms or bar structure readily discernible. It exhibits a slightly elliptical shape, appearing somewhat flattened but not highly elongated. The color profile suggests a predominantly older stellar population, with a redder overall hue. There is a faint hint of bluer regions possibly indicating a low level of on-going star formation activity, however, the bulk of the light seems to originate from evolved stars. No signs of major mergers or tidal disruptions are visible. There is a very slight asymmetry, with a possible minor disturbance. The overall appearance is consistent with an early-type galaxy, likely a lenticular or elliptical galaxy with a substantial mass, that is relatively quiescent in terms of star formation.
