The galaxy presents a generally smooth morphology. The central region exhibits a bright, slightly elliptical core with a yellowish-white hue, suggesting a concentration of older stellar populations. Fainter, bluish-white extensions are visible to the left of the core, hinting at possible disk-like structures or tidal features. The overall color distribution appears to be relatively uniform, with a slight shift towards bluer tones in the aforementioned extensions. Indications of potential minor disturbances are also visible in the outer regions. These disturbances, along with the aforementioned features, suggest that there may be a possibility of a recent or ongoing merger event. 
