The galaxy presents as a smooth, elliptical structure with a concentrated central bulge. The galaxy exhibits a general yellowish hue, indicative of an older stellar population. The light distribution is centrally concentrated. The galaxy appears relatively undisturbed, with no obvious signs of major merging activity or significant tidal features. Its elliptical shape suggests a relatively high degree of rotational symmetry. Faint hints of bluer regions are visible on the outer edges of the galaxy, potentially indicating regions of more recent star formation, although these features are subtle.
