The galaxy presents as a relatively concentrated object with an elliptical morphology. A prominent, bright central bulge dominates the luminosity profile. There appears to be a tidal tail or plume extending from the main body of the galaxy, suggesting ongoing or recent gravitational interaction with another galaxy. The color of the central bulge is yellowish, indicative of an older stellar population. There appears to be some level of disturbance, which is likely due to an ongoing merger.
