The galaxy exhibits a predominantly smooth morphology with an approximate angular radius of 2.5 arcseconds. The light profile appears relatively even, lacking a strong central bulge or well-defined spiral arms. However, there seems to be a significant amount of disturbance or recent interaction, with a possible merger. There seems to be minor disturbances in the structure of the galaxy.

Color analysis reveals a blue hue in the central region, likely indicating the presence of young, hot stars. The outer regions appear redder, possibly indicating an older stellar population. The galaxy shows signs of a possible merging event, with a light disruption in the top center of the galaxy.
