The galaxy presents as a moderately bright, elliptical object with a concentrated central bulge. The light distribution appears smooth, with the luminosity decreasing gradually from the center outwards, suggesting an older stellar population. The galaxy exhibits a flattened shape, appearing somewhat elongated along one axis. There is no evidence of spiral arm structure or prominent dust lanes within the galaxy. Faint color variations hint at differences in the stellar populations between the core and the outer regions. Overall, the galaxy appears well-formed and undisturbed, without noticeable tidal features or signs of recent merger activity.
