The galaxy appears to be a relatively smooth, centrally concentrated object with an elliptical morphology. There is little evidence of spiral arm structure or significant dust lanes. The light distribution suggests an older stellar population, with a color profile that is generally redder, indicating a lack of ongoing, significant star formation within the galaxy. The galaxy is slightly elongated and exhibits a high Sersic index, further supporting its classification as an elliptical galaxy. There is a suggestion of a faint halo surrounding the core. Overall, the galaxy is a relatively quiescent system, and there is no evidence of any strong interaction or merging activity.
