The galaxy presents a generally smooth morphology. It is somewhat elliptical in shape, displaying a moderate degree of elongation. The light distribution appears to be centrally concentrated, with a gradual decrease in brightness towards the outer regions. There is a hint of a possible interaction or minor disturbance, perhaps indicative of tidal features or an ongoing merger with a smaller companion. Overall, the galaxy does not exhibit strong features associated with active star formation, suggesting a relatively quiescent or passive nature. The color appears to be typical of aging stars in a population.
