The galaxy presents as a centrally concentrated object, likely elliptical in morphology. A dominant, luminous bulge is evident, exhibiting a smooth, almost featureless appearance. The galaxy displays a nearly circular form, with minimal deviation from radial symmetry. There's a hint of a very faint, diffuse halo surrounding the central region. Overall, the galaxy lacks prominent spiral arm structures or strong indications of active star formation, suggesting an older stellar population. There may be signs of a minor gravitational interaction present, as there appear to be subtle disturbances in the outskirts of the galaxy.
