The galaxy appears to be a disk-shaped system, exhibiting a moderate degree of inclination relative to our line of sight. The central bulge is prominent and appears yellowish, suggesting a population of older stars. Faint spiral arms may be present but are poorly defined, potentially due to limited resolution or the galaxy's type. The overall color gradient indicates a redder center and slightly bluer outer regions, hinting at some ongoing star formation in the disk. The galaxy's morphology is primarily smooth in appearance. There is no readily apparent evidence of a major merger or significant tidal disturbances.
