The galaxy presents as a relatively smooth, elliptical morphology. There is a slight elongation, deviating from a perfectly circular form, with no apparent prominent disk structure or spiral arms. The galaxy displays a concentrated central bulge that appears to be quite old, based on color. No signs of major mergers or significant tidal disturbances are visible. The overall color suggests an older stellar population, with a relatively low ongoing star formation rate. The galaxy's size is relatively compact.
