The galaxy appears as a centrally concentrated, elliptical-like structure with a smooth light distribution. It exhibits a moderately elongated shape, with the major axis notably longer than the minor axis. There is a subtle color gradient visible, transitioning from a bluer hue in the central region to slightly redder tones towards the outer edges. This galaxy shows no indication of spiral arms or prominent dust lanes and no signs of recent major merging activity, although there might be minor disturbances from a past event. Based on its overall morphology and color profile, it appears to be a relatively evolved system with ongoing star formation and an intermediate mass.
