The galaxy appears to be a relatively smooth, elongated elliptical galaxy. There is no obvious spiral structure or strong disk component visible. The light is concentrated towards the center, with a gradual decrease in brightness outward. The galaxy's color suggests an older stellar population; the core appears slightly more yellow, indicative of evolved stars. There is some indication of possible minor disturbances, which is likely due to the early stage of a minor merger or some faint tidal tails. Overall, this appears to be a reasonably massive galaxy, consistent with an early-type classification.
