The galaxy presents as a primarily smooth, elliptical morphology. Its light is concentrated towards the center, exhibiting a bright, well-defined nucleus, which suggests a high stellar density. The galaxy's overall color appears to be on the redder side, indicating an older stellar population with minimal ongoing star formation. There are no obvious spiral arm structures or dust lanes visible. The galaxy appears largely undisturbed, showing no signs of major mergers or tidal distortions. A very faint and subtle halo of light seems to surround the central region, suggesting a gradual decline in stellar density outwards.
