The galaxy presents as a mostly smooth, elliptical-like structure. It appears fairly symmetric, with a high degree of central concentration. The galaxy exhibits a distinct roundness in its shape and a minimal presence of disk-like features. There is no strong evidence of significant ongoing or recent merger activity based on the galaxy's overall morphology. The light distribution is concentrated towards the central region, with a relatively smooth decline in intensity moving outward. The color profile is dominated by redder hues, indicating an older stellar population, with some bluer regions.
