The galaxy exhibits an elliptical morphology, appearing largely smooth and spheroidal with a high degree of central concentration. There is no apparent disk structure or spiral arm features. The color profile suggests an evolved stellar population, exhibiting a reddish-yellow hue. The galaxy's light appears to be dominated by older stars. A faint extended halo appears to surround the central, brighter region, possibly indicating a more diffuse stellar population. There is a slight irregularity in shape that may be due to a tidal interaction or minor merger event, or some internal disturbance, though the galaxy appears largely unperturbed. Overall the galaxy appears to be a relatively massive, quiescent system.
