The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a moderate degree of ellipticity, appearing more 'in between' round and cigar-shaped. The central region displays a bright, concentrated core. There is no clear evidence of spiral arms or a prominent disk structure. The color profile suggests a population of older stars, with a slightly redder hue. No major disturbances or mergers are apparent in its immediate vicinity, though there may be minor disturbances. The galaxy is a fairly large, massive galaxy. Overall, the observed characteristics point towards a galaxy with a substantial spheroidal component and limited ongoing star formation.
