The galaxy presents a generally smooth, elliptical morphology, with a bright, concentrated central bulge. It exhibits a flattened, disk-like structure, although features are not clearly resolved. The colour gradient suggests a population of older stars, particularly within the central region, indicated by the yellowish hue. Some localized areas of increased luminosity are present along the galaxy's plane, which may suggest regions of enhanced star formation, or could also be the result of image artifacts. There is no obvious evidence of a major ongoing merger or significant tidal disturbance from this observation.
