The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The light distribution is somewhat elongated, deviating from a perfectly circular profile. The dominant color is reddish-yellow, suggestive of an older stellar population and minimal ongoing star formation. The galaxy appears to be experiencing some form of gravitational disturbance, possibly due to a minor merger. There is a slight asymmetry in its outer regions. There are regions of increased light near the center of the galaxy.
