The galaxy exhibits a primarily elliptical morphology, though some distorted features are visible. The central region displays a high degree of luminosity, with a concentration of older stellar populations exhibiting a yellowish hue. There is evidence of potential tidal disturbances or ongoing merger activity, indicated by a faint, elongated extension or tail emanating from the main galactic body. The overall structure appears somewhat irregular, possibly due to gravitational interactions with another galaxy. Star formation appears to be relatively low within the galaxy. The galaxy is not perfectly spherical; it appears slightly elongated along one axis.
