The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in surface brightness towards the outer regions. There are no visually discernible spiral arm structures. The galaxy appears largely featureless, lacking prominent dust lanes or distinct star-forming regions. The overall color is consistent with a population of older stars, suggesting relatively low current star formation activity. The isophotes appear relatively round. There's no strong indication of ongoing or recent merger events based on visual distortions or tidal tails. There is a small amount of disturbance indicated, however, it is hard to visually identify the source of this from this image. Overall, the galaxy seems to be a well-formed elliptical galaxy.
