The galaxy exhibits a morphology that appears disturbed, possibly indicative of a recent or ongoing merger event. The light distribution is not smooth; there are several distinct clumps or concentrations of luminosity. The primary body of the galaxy has an elongated shape. There is a notable redder region towards the apparent lower portion of the galaxy. The overall color suggests an older stellar population with lower star formation activity, though the clumps may indicate pockets of more recent star formation. There may also be a tidal tail emerging from the galaxy, further supporting the hypothesis of an interaction with another galaxy.
