The galaxy presents a predominantly smooth morphology. It exhibits a central, concentrated bulge that appears yellow-white, indicating an older stellar population. Fainter, bluish light surrounds this central region, suggesting the presence of a disk component with some ongoing star formation. Irregularities in the light distribution of the outer disk hint at possible disturbances, potentially due to past minor mergers or tidal interactions. Although a defined spiral structure is not readily apparent, the overall shape leans toward a disk-like structure rather than a purely elliptical one. There appears to be evidence of possible past merger events or gravitational disturbance.
