The galaxy presents a generally smooth and centrally concentrated morphology. There's evidence of a slight flattening, moving it away from being a perfect circle. It exhibits a dominant central bulge that appears bright and somewhat diffuse, possibly indicating a high concentration of older stars. The galaxy's overall color is slightly yellow, suggesting an older stellar population and reduced recent star formation. A very slight asymmetry or disturbance might be present in its outer regions. There is no evidence of spiral arm structure or significant dust lanes. Overall, the galaxy appears to be a relatively quiescent system, with a smooth light distribution and subdued star formation.
