The galaxy presents as a single, largely featureless object, with an overall elliptical morphology. The light distribution appears smooth and concentrated toward the center, indicating a likely evolved stellar population. The galaxy exhibits a color gradient, appearing yellower and redder towards the central region. This suggests the presence of older, redder stars concentrated towards the core, possibly due to a lack of recent star formation activity in this region. The outer regions of the galaxy are dimmer and appear somewhat bluer, possibly indicating a younger stellar population. The shape of the galaxy is mostly round. There is no visual indication of strong tidal interactions or major mergers. Possible minor disturbances could be present, but it is hard to say.
