The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal. The light distribution suggests a centrally concentrated luminosity profile, indicative of an older stellar population. There is a slight elongation, deviating from a perfectly circular form. No distinct spiral arms or prominent dust lanes are discernible. The galaxy's color appears generally uniform, with a yellowish-white hue suggesting a lack of significant ongoing star formation. There is no apparent evidence of recent or major merger events. The galaxy appears relatively undisturbed.
