The galaxy presents as a disk-shaped system, viewed at an oblique angle. There's evidence of a central bulge, characterized by a concentrated region of relatively even light distribution. Extending from the central region, the disk exhibits a mottled texture, suggesting a non-uniform distribution of stellar populations and dust. There appears to be a disturbance in the upper portion of the galaxy, where one part of the disk region curves slightly away from the rest of the galaxy, and an area of the disk appears more dispersed. Its overall color indices suggest a mix of young and old stellar populations, with hints of ongoing, though potentially subdued, star formation.
