The galaxy presents as a somewhat diffuse, elliptical-like structure, elongated along a major axis with an estimated axis ratio indicating a flattening. The light distribution is centrally concentrated, showing a smooth gradient outwards from a brighter core region. The overall color appears bluish, suggesting the presence of a population of relatively young, hot stars, particularly in the central regions. There is no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy exhibits a gradual decrease in surface brightness with increasing radius, with a well-defined edge. A slight asymmetry may be present.