The galaxy presents a predominantly smooth morphology. The central bulge appears to be relatively prominent and exhibits a reddish hue, suggesting a population of older stars. Surrounding the bulge, there's a disk-like structure with a slightly bluer tint, possibly indicating ongoing star formation. There's a subtle suggestion of spiral arms, but they are not clearly defined. Faint disturbances, like tidal tails or asymmetric features are subtly present, suggesting possible minor gravitational interaction with a nearby object. The galaxy is generally round.
