The galaxy presents as a slightly elongated, lenticular-like structure with a smooth, centrally concentrated luminosity profile. The core exhibits a bright, yellowish hue, suggestive of an older stellar population. There is a subtle color gradient, with the outer regions appearing marginally bluer than the core, which may indicate some ongoing, though limited, star formation in the outer disk. The overall smooth appearance suggests a lack of significant spiral arm structure or prominent dust lanes. There is no immediately apparent evidence of a major merger event, though subtle disturbances in the outer halo cannot be completely ruled out given the image resolution. Its angular size is relatively compact, implying considerable distance. Based on its morphology, the galaxy is most likely a relatively massive system.
