The galaxy presents as a primarily smooth, elliptical structure. The central region exhibits a concentrated, bright yellowish-white luminosity, indicative of an older stellar population. The overall shape appears somewhat rounded, verging on elliptical. Faint extensions of diffuse blue light are visible on either side of the central bulge, suggesting the presence of some younger star formation regions within what may be the remnants of a disk. No obvious signs of tidal tails, major mergers or significant disturbances are apparent, although there may be minor disturbance to one side. The galaxy possesses a relatively high mass and low star formation rate.
