This galaxy exhibits a generally smooth morphology, with a discernible central bulge. The overall shape appears somewhat elliptical, though with slight deviations from perfect roundness. While a dominant spiral arm structure is not evident, there is a suggestion of faint, diffuse disk-like features.

Color gradients across the galaxy indicate a possible variation in stellar populations or dust content. The central region appears to be a reddish-yellow, potentially indicative of older stellar populations. The outer regions of the galaxy display hints of bluer hues, suggestive of the presence of younger, hotter stars.

There is an apparent lack of significant tidal tails or other morphological disturbances. The faint indications of ongoing star formation are noted.
