The galaxy presents a flattened, elliptical morphology. A central bulge appears bright and yellowish, suggesting a population of older, redder stars. Extending outwards from the central region, a fainter disk is visible. The disk exhibits subtle color variations, with hints of bluer regions suggestive of ongoing, but low, star formation activity. The overall structure does not show any major disturbances or signs of on-going merging events, however there may be some minor disturbances that are not as visible. The galaxy appears to be relatively isolated.
