The galaxy presents a somewhat irregular morphology, appearing neither fully elliptical nor exhibiting a well-defined spiral structure. A dominant central bulge, exhibiting a yellowish hue, suggests a significant population of older stars. Fainter, bluer patches are observed extending from the central region, possibly indicative of ongoing star formation. There is a distinct blue region to the left that may indicate that the galaxy is interacting with it. Overall, the galaxy appears relatively compact, with a smooth appearance.
