The galaxy presents as a largely featureless, elliptical-like structure with a smooth light distribution, indicating a high degree of sphericity. The central region exhibits a significantly higher surface brightness than the outer regions, suggesting a concentrated stellar population. The galaxy displays a color gradient, appearing bluer toward the center and becoming progressively redder in the outer regions. This may indicate a difference in stellar populations, with younger, bluer stars being more concentrated towards the center, and older, redder stars dominating the periphery. There are no prominent spiral arms or dust lanes visible. No evidence of significant tidal disturbances or ongoing major mergers is apparent.
