The galaxy presents an overall smooth appearance, with a dominant, spheroidal central bulge that exhibits a concentrated, bright core. The light distribution suggests a relatively old stellar population dominating the bulge. There is faint disk structure visible beyond the bulge, which are slightly irregular and diffuse. The color gradient transitioning from the core to the outer regions shows a slight bluer trend, which is consistent with ongoing star formation in the disk compared to the bulge. Additionally, a faint plume or tidal feature extends from the main body of the galaxy, indicating a possible recent interaction or merger event. The overall morphology suggests a galaxy in transition, possibly evolving from a spiral to an elliptical type through mergers and internal processes.
