The object presents as a moderately sized galaxy. Its overall morphology appears to be that of a disk galaxy with a degree of disturbance. There appears to be a merger or tidal interaction occurring, indicated by the lopsided and irregular shape. The central bulge region is somewhat condensed, but not entirely smooth; potential dust lanes or other substructures exist within it. There is evidence of faint disk-like features extending beyond the brighter central region. The color gradient suggests ongoing star formation, though it doesn't appear to be dominant, but there may be a presence of intermediate-age stellar populations along with older populations contributing to the overall light. There may be a faint tidal tail indicating that the galaxy has undergone a merger in the past, or is currently merging with another, smaller object that cannot be easily seen.
