The galaxy presents as a relatively smooth, centralized structure with minimal discernible spiral arm features. Its overall shape tends towards round, though not perfectly spherical. There is evidence of some minor disturbances and an irregular distribution of light within the galactic disc, possibly indicating past or ongoing interactions. The galaxy's color appears relatively uniform and consistent, with the suggestion of a higher concentration of older stellar populations and subdued ongoing star formation. The galaxy's apparent size is reasonably compact, suggesting a moderate physical dimension.
