The galaxy presents a generally smooth morphology. The object is a slightly elongated spheroid, exhibiting a centrally concentrated luminosity profile. The core region appears bright and compact, with the light gradually fading towards the outer edges. There is a slight suggestion of a flattened structure indicative of a disk component, although the overall smoothness indicates that it may be a lenticular galaxy, rather than a spiral. Faint blue hues are visible within the galaxy's structure, suggestive of some degree of ongoing star formation, though likely at a subdued rate. No distinct spiral arms or prominent dust lanes are visible. There is very faint indication of tidal interactions or disturbances, though the galaxy looks relatively undisturbed.
