This galaxy presents as a largely featureless elliptical type. It exhibits a concentrated, bright core region, with luminosity decreasing radially outwards. The color profile suggests an older stellar population, with a reddish-gold hue dominating the central region, possibly indicating a prevalence of evolved stars. The overall shape is approximately circular, though a slight elongation is possibly discernible. There are faint, diffuse extensions beyond the core, though no distinct spiral arms or other clear morphological features are visible. There appears to be some minor disturbances in the outer regions that could indicate a past or ongoing merger event. The galaxy appears relatively isolated.
