The galaxy presents as a singular, centrally concentrated object, demonstrating a smooth morphology. It exhibits a predominantly elliptical or spheroidal shape, with a high degree of roundness. The color profile of the galaxy skews towards the red end of the spectrum, indicating a stellar population dominated by older, redder stars. There appears to be no discernible spiral arm structure or prominent dust lanes, which further supports the classification as an elliptical or lenticular galaxy. The galaxy displays a homogenous, relatively undisturbed structure, with no obvious signs of tidal interactions or recent major mergers. There is a slight suggestion of some disturbance, but it appears to be more in the minor category. The galaxy shows indications of star formation activity.
