The galaxy presents as an irregular system, exhibiting evidence of ongoing or recent merger activity. The overall structure appears disturbed, with a prominent tidal tail extending from the main body, suggesting gravitational interaction with another galaxy. The central region appears smooth, but not entirely featureless, as a slight elongation is noted. The light distribution is concentrated, indicating a dense core, however the overall shape appears in between round and cigar shaped. Multiple components are observed that could be remnants of galaxies that merged to create it or it could be multiple star forming regions. The color profile is indicative of a potentially high star formation rate.
