The galaxy presents a primarily smooth morphology, with a notable absence of distinct spiral arms or prominent substructures. It exhibits a somewhat elongated shape, appearing more "in-between" round than a perfect circle. The central region displays a concentrated luminosity, with the light gradually decreasing towards the outer edges. The overall color profile appears to be relatively red, suggesting a stellar population dominated by older stars and a low ongoing star formation rate. There are no immediately apparent signs of major disturbances or ongoing merger activity, although some minor irregularities in the outer regions cannot be entirely ruled out. The galaxy's smooth appearance and redder color indicate that it is likely a relatively massive system.
