The galaxy presents as an elliptical morphology. It appears mostly smooth in texture, with no apparent spiral arms or bar structures visible. The galaxy is characterized by a central, concentrated region of intense light, suggesting a high stellar density at its core. The light profile diffuses outwards from the center in a smooth gradient, indicative of a relatively homogenous stellar population. The overall color of the galaxy appears slightly redder, indicating a population of older stars, thus it is consistent with it being an older galaxy. No obvious signs of ongoing major merger events or significant tidal disturbances are observed; however, closer analysis may be warranted to check for minor disturbances.
