The galaxy presents as a somewhat smooth, elliptical-like structure, with a slight elongation suggestive of a transition between a round and cigar-shaped morphology. Its central region appears concentrated and bright, fading gradually into a diffuse halo. There are faint hints of internal structure, but no prominent spiral arms or bar features are discernible. The galaxy appears relatively isolated, exhibiting only minor disturbances. The overall color suggests a population dominated by older stars, with little evidence of active star formation.
