The galaxy presents as a centrally concentrated object with a generally smooth morphology. The primary light emission appears yellowish-white, indicative of a primarily older stellar population. The galaxy exhibits a near-spherical or slightly elliptical shape, showing a lack of defined spiral arms or a prominent disk structure. There are faint blue tinges within the surrounding, less dense galactic halo. The light distribution is relatively smooth and the edges of the halo seem fuzzy. There is no visible evidence of ongoing major mergers or tidal disturbances. The galaxy is estimated to be of intermediate mass, and observations suggest a relatively low rate of star formation.
