The galaxy presents a generally smooth and centrally concentrated morphology. It appears elliptical in shape, with the light distribution gradually decreasing from a bright core. There is little evidence of spiral arms or a distinct disk structure. The galaxy exhibits a relatively uniform color gradient, transitioning from a bluer central region to redder outer edges. There is a suggestion of minor disturbances in the overall shape, but no prominent signs of ongoing major mergers or strong tidal interactions are observed.
