The galaxy presents as a relatively smooth, elliptical morphology. The light distribution is concentrated toward the center, exhibiting a bright, prominent core indicative of an older stellar population. The galaxy appears somewhat rounded in shape, with only a slight deviation toward a more elongated form. There is no clear evidence of spiral arm structure or ongoing major mergers. Faint, diffuse light extends outwards from the core, forming a halo that fades gradually into the background. No significant dust lanes or patches are readily apparent. Minor disturbances may be present, but these are not visually dominant features. The overall color appears to be yellowish-red. Star formation appears to be present but not dominant.
