The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a high degree of luminosity, suggesting a concentrated nucleus. A slight elongation is apparent, deviating from a perfect circular shape. Faint, diffuse structures are visible in the outer regions, indicating the potential presence of a disk or tidal features, though these features appear subdued. The galaxy's overall color is dominated by warmer hues, transitioning to cooler tones toward the periphery. There is no prominent evidence of ongoing major merging activity, but the subtle disturbances could indicate a past or ongoing minor interaction.
