The galaxy presents as a single, cohesive object with a predominantly smooth morphology. Its shape is largely round, though some slight elongation is noted. The color appears yellowish orange, suggesting an older stellar population. Evidence of any distinct disk-like structure is faint. There is no clear sign of major merging activity, but subtle disturbances or interactions might be occurring. Overall, the system appears to be a relatively undisturbed elliptical galaxy or a lenticular galaxy with a small disk at a significant distance.
