The observed galaxy presents a morphology consistent with a relatively compact object. It exhibits a central, bright core, surrounded by a diffuse halo of lower surface brightness. The color profile suggests a blue-green hue in the central region, transitioning to a redder tint towards the outer edges. This could indicate a population of younger, hotter stars concentrated towards the center, with older, cooler stars dominating the outskirts. There appear to be potential signs of minor tidal disturbances or interactions, evidenced by slight asymmetries in the halo structure. There is a marginal indication of possible merging activity. The overall structure indicates a potentially smooth, though possibly dynamically perturbed galaxy.
