The galaxy appears to be a smooth, elliptical galaxy with a hint of a disk structure. It exhibits a yellowish-red hue overall, suggesting an older stellar population. The galaxy's shape is somewhat elongated, appearing somewhere between round and cigar-shaped. There is no clear evidence of any major merging activity or significant tidal disturbances, though a minor disturbance cannot be completely ruled out. Based on its color, size, and general morphology, this galaxy has likely ceased much of its star formation and is primarily composed of older stars.
