The galaxy presents as an elliptical morphology, appearing largely smooth and relatively featureless at this resolution. Its central region exhibits a concentrated luminosity profile, with a yellow-orange hue indicative of an older stellar population. The galaxy's apparent shape tends towards roundness, with a subtle elongation. There is no discernible evidence of significant tidal disturbances, merging activity, or a prominent disk structure. The light distribution suggests a system dominated by evolved stars with relatively low current star formation. The galaxy's structure shows a slight deviation from perfect symmetry, but it mostly presents as a relaxed and settled system. 
