The galaxy presents a generally smooth, elliptical morphology. It displays a concentrated, bright central bulge that transitions smoothly into a fainter, more diffuse halo. There is no clear evidence of spiral arms or a distinct disk structure. The color gradient suggests a population of older stars dominating the galaxy's composition, with a higher concentration of these older, redder stars in the central bulge. There are no strong indications of active star formation regions or dust lanes within the galaxy. There are no clear signs of any ongoing major merging events, however, there is a slight possibility of minor tidal disturbances or interactions. The overall form appears fairly relaxed and undisturbed.
