The galaxy appears to be an elliptical galaxy, characterized by a smooth, spheroidal morphology and a dominant central bulge. The central region exhibits a yellowish hue, likely indicating an older stellar population with a lower rate of star formation. This core gradually transitions into a more greenish outer halo, suggesting the presence of some younger stars or possibly ionized gas, although the overall star formation activity is relatively low. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy does not appear to be undergoing any major merging activity, although there are some subtle irregularities in its outer regions that suggest a possible minor gravitational interaction. The shape of the galaxy is generally ellipsoidal with the ratio of the minor to major axis being less than 1.
