The galaxy presents as a relatively small, elliptical or lenticular system, seen nearly face-on. The core is bright and concentrated, exhibiting a smooth light profile with a yellowish-white hue, indicative of an older stellar population. The surrounding halo appears fainter, transitioning into a blueish color, suggesting the presence of a younger stellar population. There is no readily apparent spiral structure or significant dust lane. The overall morphology suggests the galaxy is relatively undisturbed, with no signs of recent major mergers. A slight asymmetry may hint at a minor interaction. Its size is consistent with a galaxy of moderate mass. The faint blue tinge suggests a low level of ongoing star formation.
