The galaxy appears as a centrally concentrated, somewhat elliptical structure. It displays a relatively smooth, diffuse light distribution, with a bright yellowish core. There are hints of fainter, slightly bluer, extended regions surrounding the core, possibly indicating a faint disk or halo component. The overall color suggests a population of older stars, though the subtle bluer regions may imply some ongoing star formation. There is slight visual evidence of a minor disturbance in the galaxy's morphology, but it mainly appears relaxed and stable.
