The galaxy appears as a roughly circular, centrally concentrated object. The light distribution suggests a primarily smooth morphology, but with some subtle irregularities hinting at possible faint features or disturbances. There is no obvious spiral arm structure present. The galaxy's light profile shows a fairly concentrated core, with light intensity gradually decreasing towards the outer edges. The color appears relatively uniform across the galaxy, indicating a potentially homogenous stellar population or dust distribution. However, the image quality limits detailed color analysis. Overall, based on visual inspection, the galaxy appears to be a relatively undisturbed, spheroidal galaxy.
