The galaxy presents a generally smooth morphology, with a slight deviation from perfect sphericity. The light distribution suggests a concentrated central bulge that fades into a more diffuse halo. There is a subtle suggestion of a disk structure, though it is not a prominent feature. The galaxy appears to be undergoing some form of interaction, the morphology is heavily disturbed, appearing to be in a late stage merger. This conclusion is supported by the irregular light distribution and distorted shape of the galaxy. The overall color suggests an older stellar population, but some bluer regions could indicate pockets of recent or ongoing star formation. The overall structure points towards a relatively evolved system with evidence of past or current interactions shaping its form.
