This galaxy exhibits a primarily smooth morphology, with a notable disk-like structure. The central region presents a bright, concentrated core, suggesting a substantial stellar population. The overall shape is somewhat elongated, deviating from a perfectly circular form; more cigar shaped than round. Faint, diffuse extensions are observed emanating from the main body, which could indicate tidal features, past minor interactions, or ongoing star formation activity within the disk. Overall, the galaxy appears to be a relatively massive system with a moderate star formation rate.
