This galaxy presents a generally smooth morphology, although it is not perfectly symmetrical. The central region exhibits a bright, concentrated luminosity. The light profile appears relatively uniform moving outwards from the center, without strong evidence of spiral arms. A subtle disturbance in shape can be observed on the left side of the galaxy, perhaps indicating a minor interaction or internal asymmetry. The overall color suggests a mixed population of stars, but with a relatively high fraction of older stars. There is a possibility of past or ongoing minor merger activity influencing its morphology.
