The galaxy presents an elliptical morphology, with a high degree of central concentration. There is a smooth transition in luminosity from the bright central bulge to the outer regions. The isophotes appear to be relatively regular with an axis ratio that is approximately 0.7, indicating an oblate shape. The galaxy is not perfectly circular, having an ellipticity that departs from a spherical distribution. The major axis is oriented at approximately 80 degrees with respect to the horizontal. There is no apparent structure such as spiral arms or bars visible. The color gradient suggests a population of older stars within the bulge. No tidal features or prominent dust lanes are visible.
