The galaxy presents an overall elliptical shape, though the disk is somewhat pronounced. It appears relatively compact and the light is concentrated, suggesting a moderate surface brightness. Some asymmetry is noticeable within the galaxy's structure. A faint, diffuse halo surrounds the central region, extending outwards. The galaxy's core exhibits a bright and concentrated intensity. There is evidence of potential minor disturbances and/or faint tidal features, which are subtle but may indicate past interactions or mergers. Overall, the galaxy appears to be relatively smooth, with no prominent spiral arms or features of active star formation immediately obvious.
