The galaxy presents an elliptical morphology, appearing significantly elongated. The light profile suggests a smooth distribution, lacking prominent spiral arms or other distinct features. There is a slightly brighter, more concentrated region towards the center, suggestive of a galactic nucleus. Color gradients are subtle, with a possible shift toward bluer hues in the outer regions, potentially indicating younger stellar populations relative to the core. No evidence of tidal disturbances or ongoing mergers is readily apparent. The galaxy appears relatively isolated.
