The galaxy presents a generally elliptical morphology, appearing more elongated than circular. A smooth light distribution characterizes its central region, with a gradual decline in brightness towards the outer edges. While difficult to discern at this resolution, there may be some faint indications of a disk-like structure. The color profile reveals a higher concentration of redder hues in the central bulge, suggesting an older stellar population residing in the core. The outer regions exhibit bluer tints, potentially indicative of younger stars. The overall structure suggests a galaxy undergoing a transitional phase, possibly evolving from a disk galaxy to a more elliptical system, or a system with ongoing minor disturbances or a merger event in progress.
