The galaxy presents as an elliptical or lenticular system, exhibiting a generally smooth and rounded morphology. There is a lack of readily discernible spiral arm structure or prominent dust lanes. The galaxy appears to be centrally concentrated, with a gradual decrease in luminosity towards its outer edges. No significant signs of tidal disturbances, major mergers, or intense star-forming regions are immediately apparent, suggesting that it is likely an evolved system. The overall color suggests a population of older stars, implying a relatively low star formation rate.
