The galaxy appears as a centrally concentrated, ellipsoidal system with a smooth morphology. Its color profile suggests a moderate stellar population age, with a likely mix of both older, redder stars dominating the core and a younger, bluer population in the outer regions. The galaxy's shape is elongated, but not strongly so. There's no obvious indication of spiral arm structures or significant dust lanes. The galaxy seems relatively undisturbed, showing no signs of a major merger event or strong tidal interactions. Minor disturbances cannot be ruled out however. The overall impression is that of an intermediate-mass, relatively quiescent galaxy at a considerable distance.
