The galaxy presents as an elliptical morphology, appearing generally smooth in structure without prominent spiral arms or a well-defined disk. The light distribution appears concentrated towards the center. Color gradients are subtle, but the core region exhibits a yellower hue, suggesting a population of older stars and/or a higher concentration of dust. The outer regions show a slight shift towards redder tones. Overall, the galaxy appears relatively undisturbed, lacking significant signs of ongoing mergers or tidal interactions. There may be a very slight deviation from perfect ellipticity, possibly due to the early stages of a minor interaction or internal kinematic processes.
