The galaxy presents a generally smooth morphology, with a high probability of being categorized as smooth rather than featuring prominent spiral arms or a distinct disk. The galaxy's shape appears to be somewhere between round and elliptical. The color distribution suggests an older stellar population, with a redder overall hue dominating the observed light. There is little evidence of active star formation regions; however, the galaxy does not look completely quiescent, as there are small areas of blue light present within. The galaxy does not show strong signs of a major merger event in its recent past. Faint hints of tidal disturbances suggest the possibility of minor interactions or past mergers.
