The galaxy presents a generally elliptical morphology. Its light distribution appears relatively smooth and concentrated, indicating an evolved stellar population. There are no visible signs of spiral arms or active star formation regions, but there are some minor irregularities in its structure. The galaxy shows a dominant, spheroidal component with an absence of distinct features, such as a bar or ring structure. The galaxy's color suggests it is comprised of older, redder stars, with low specific star formation rate. The round fraction indicates that its ellipticity is not extreme. There is little evidence of any significant mergers or tidal interactions, though there is minor disturbance.
