The galaxy presents as a largely smooth, centralized structure with a high degree of ellipticity. A bright, concentrated core dominates the visual appearance, surrounded by a more diffuse, extended halo. The color gradient indicates a potential change in stellar population or dust content from the core to the outer regions. There is evidence of some disk structure. There appears to be signs of some minor disturbances in the galaxy's morphology, although it is not undergoing any significant merging activity.
