The galaxy appears to be an elliptical galaxy with a smooth, relatively featureless morphology. It exhibits a generally ellipsoidal shape, appearing elongated with an approximate axis ratio of perhaps 3:1. The light distribution is concentrated towards the center, suggesting a high degree of central mass concentration. There is a slight color gradient, with the central region appearing more yellow/orange and the outer regions exhibiting bluer tones. This color differential could indicate a difference in stellar population, with older, redder stars dominating the core and younger, bluer stars populating the outer regions. There's no obvious evidence of spiral arms, dust lanes, or any significant ongoing merging activity. Overall, the galaxy seems to be a relatively undisturbed system, displaying properties consistent with a mature elliptical galaxy.
