The galaxy presents as a single, diffuse object with a notable degree of smoothness. The overall shape appears to be elliptical or lenticular, as there is no evidence of spiral arm structures. The galaxy exhibits a central concentration of light that gradually diminishes towards the edges. Color gradients appear subtle but present, with the core region exhibiting a slightly yellower or redder hue, suggesting a population of older stars. The outer regions appear slightly bluer in comparison, potentially indicating the presence of younger stellar populations or ongoing star formation, although these are not readily apparent. The galaxy does not appear to be undergoing any major mergers or interactions, with no significant tidal tails or distortions visible. The overall morphology suggests a relatively relaxed and evolved system.
