The galaxy exhibits a relatively compact morphology. A bright, centrally concentrated core is observed, surrounded by a fainter, more diffuse halo. The light distribution appears largely smooth, with no obvious spiral arm structures or prominent dust lanes visible. However, there are suggestions of minor disturbances or irregularities in the outer regions. A subtle deviation from perfect elliptical symmetry is noted, possibly indicating a past or ongoing interaction with another galaxy, or internal dynamical processes. There are red regions observed in the galaxy, particularly around the bright center, and in a fragmented fashion in the outer regions. A green ring encompasses the bright center. The overall color suggests a mix of stellar populations, with a noticeable contribution from older, redder stars, as well as the presence of younger, bluer stars in the central core.
