The galaxy appears as a roughly circular, smooth structure with a concentrated central bulge. The overall color is yellowish-orange, suggesting a population of older stars, with a potential absence of ongoing, significant star formation. There is a lack of discernible spiral arms or a prominent disk structure. The light distribution fades gradually from the core outwards, indicating a relatively uniform stellar population. The galaxy does not exhibit any obvious signs of tidal disturbances, major mergers, or active galactic nuclei activity based on the available image.
