The galaxy presents a moderately bright, somewhat elliptical morphology. Its central region exhibits a concentrated, yellow hue, suggesting a population of older stars. A slightly fainter and bluer disk component is also present, extending outwards from the central bulge. The galaxy shows hints of spiral structure, though these features are somewhat diffuse and lack distinct arm definition. Overall, the galaxy seems to be in a relatively quiescent state, with a moderate level of star formation.
