The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is a hint of disk structure and potentially spiral arm features, however, the smoothness of the overall light profile suggests a significant bulge component. The galaxy displays a noticeable color gradient, with a bluer core transitioning to redder outer regions. This color variation could indicate ongoing star formation activity in the central regions and a more aged stellar population in the outer regions. There's a potential indication of a minor disturbance in the galaxy's morphology, which may be indicative of a past or ongoing interaction. However, this could also be internal processes. Overall, the galaxy appears to be relatively undisturbed with a dominant smooth component.
