The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits a predominantly elliptical or spheroidal shape, appearing largely rounded. The color profile indicates a redder hue in the central region, suggesting an older stellar population. There is a subtle indication of a disk-like structure. There are no apparent spiral arms or significant dust lanes visible in this image. No indications of tidal tails or prominent morphological disturbances suggesting a recent major merger event are observable, however a potential minor disturbance in structure or merger event may be occurring.
