The galaxy presents as a flattened, disk-shaped system, viewed at an oblique angle. The central bulge appears prominent and exhibits a smooth, concentrated light profile, suggesting a substantial population of older stars. Moving outward from the core, a faint disk is discernible, displaying a bluer color, hinting at the presence of younger stellar populations and ongoing star formation. The disk appears somewhat disturbed, possibly indicating a minor interaction or internal dynamical processes. There is no clear evidence of well-defined spiral arms; the structure of the disk seems more amorphous. Overall, the galaxy appears to be of intermediate luminosity, displaying characteristics of both spheroidal and disk galaxies, with a moderate level of star formation activity.
