The galaxy presents a generally smooth morphology, with a centrally concentrated light profile. Its shape is somewhat elliptical, exhibiting a moderate degree of elongation. A faint, diffuse halo is present, extending beyond the brighter central region. The color appears to be slightly blue-shifted towards the central region, suggestive of more active star formation in that area. No obvious spiral arm structure or significant dust lanes are discernible. There are no clear signs of any ongoing major mergers or significant tidal disturbances, although a minor interaction cannot be completely ruled out given the slight asymmetry in the outer halo.
