The galaxy presents as a relatively smooth object with a slightly elliptical morphology. There is some indication of internal structure, though the resolution is limited. The galaxy exhibits a color gradient, appearing bluer in the central regions and redder toward the outer edges. This suggests a degree of ongoing star formation in the core, with a potentially older stellar population dominating the outskirts. No significant tidal features or other indications of recent major merger events are discernible. Overall, the galaxy's morphology points towards an early-type system, possibly transitioning from a spiral to an elliptical galaxy.
