The galaxy presents as a moderately luminous object with an elliptical morphology. The light distribution appears relatively smooth and concentrated toward the center, suggesting an older stellar population. There is little evidence of spiral arms or significant dust lanes. The galaxy exhibits a slightly elongated shape, though not extremely so, appearing neither perfectly spherical nor highly flattened. There is no obvious indication of a major merger event or strong tidal disturbance impacting the overall structure. The central region appears to be a brighter yellowish hue, which suggests a concentration of older stars and a lower rate of current star formation. The outer regions appear slightly bluer and less concentrated, indicating some ongoing star formation, but at a relatively low level.
