The galaxy presents a disk-like morphology. Its apparent diameter suggests it's a relatively compact object for its class. The central bulge exhibits a bright, concentrated luminosity, indicating a potentially high stellar density or active galactic nucleus. A faint disk extends outward from the central bulge, displaying hints of spiral arm structures. The disk's color suggests a mixed stellar population, with some regions appearing bluer, possibly indicating areas of ongoing star formation, and other regions appearing redder, implying older stellar populations. The edges of the disk appear somewhat disturbed, possibly indicative of past or ongoing interactions with other galaxies. Based on light profile, the galaxy is estimated to have an intermediate mass. Star formation rate appears to be relatively low. There may be some degree of gravitational interaction with a nearby smaller galaxy to the left of the object.
