The galaxy presents a generally smooth appearance, with a centrally concentrated brightness profile. The morphology is largely elliptical, exhibiting a high degree of roundness. There is no readily apparent spiral arm structure. 

A minor disturbance is present on one side of the galaxy, but no major mergers or disturbances are visible. The galaxy core appears bright and relatively compact, surrounded by a more diffuse halo.

Colors within the galaxy show a noticeable variation; the central region exhibits a redder hue, indicative of an older stellar population, whereas the outer regions have bluer tints, suggesting more recent star formation. There is no noticeable dust lane obscuring the galaxy's structure.
