The galaxy presents as an elliptical morphology, with a concentrated, bright central bulge that is indicative of an older stellar population. There is a smoothly decreasing intensity profile moving outwards from the core, indicating a lack of prominent spiral arm structures or significant star forming regions. The galaxy has a fairly regular, rounded shape. The overall color is yellowish-red, which further supports the presence of an evolved stellar population and relatively low current star formation rate. There are no obvious signs of tidal disturbances or interactions with other galaxies.