The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution without prominent spiral arms or a distinct bar structure. The core of the galaxy appears highly concentrated with a yellowish hue, indicative of an older stellar population. Moving outward from the core, the galaxy's color transitions toward a bluer tone, suggesting the presence of younger stars in the outer regions. The overall shape appears generally spheroidal, although there may be a slight elongation along one axis. There is no apparent sign of major mergers or significant tidal disturbances in the surrounding region. The galaxy exhibits a moderate degree of star formation activity.
