The galaxy presents a generally smooth appearance. It exhibits a flattened, elliptical morphology, with a high degree of central concentration. There appears to be little to no visible disk component or spiral arm structure. The galaxy's color suggests a dominant population of older stars, with a relatively low rate of ongoing star formation. There is little evidence of significant dust lanes or obscuration within the galaxy itself. No signs of major tidal disturbances or ongoing mergers are visually apparent, although a faint asymmetry or minor perturbation within the outer regions cannot be ruled out. The overall shape indicates a relaxed system, likely an early-type galaxy or a late-type galaxy that has exhausted most of its gas supply.
