The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a slightly elongated morphology. The central region displays a concentrated luminosity, with a gradual decrease in brightness towards the outer edges. Color gradients suggest a population of older stars dominating the core, transitioning to slightly bluer hues in the outer regions, potentially indicating younger stellar populations or regions of ongoing star formation. The galaxy appears moderately inclined from our line of sight. Faint tidal features, suggesting a past or ongoing merger, can be observed. There is an area of disturbance that separates the main body of the galaxy from a smaller area that is connected by very faint tidal arms.
