The galaxy appears as a somewhat flattened, elliptical structure with a smooth and centrally concentrated light distribution. The core of the galaxy is a bright, yellowish hue, suggesting a population of older stars. The outer regions exhibit a gradual decline in luminosity and seem to have bluer tones, potentially indicating the presence of younger stellar populations in the disk. The galaxy does not appear to be undergoing any major merging activity, though there may be minor disturbances in its morphology. It has a relatively high degree of roundness, leaning towards an elliptical classification.
