The galaxy presents a largely smooth morphology, with a generally elliptical shape. It displays a noticeable bulge, centrally concentrated and exhibiting a yellowish hue, suggesting a population of older stars. Moving outward from the core, the galaxy transitions to a more greenish-blue color, possibly indicating the presence of a younger stellar population and some ongoing star formation. The overall form hints at a disk-like structure viewed at an oblique angle, although defined spiral arms are not evident. There is some subtle distortion and disruption in the outer regions, possibly indicating a minor gravitational interaction or past merger event.
