The galaxy presents as a moderately luminous, elongated structure, classified as having a notable smooth component but with some indications of disk-like or featured characteristics. The galaxy's shape deviates from a perfect sphere, appearing more as an intermediate elliptical with some elongation. There is evidence suggesting an ongoing or recent interaction, as indicated by minor disturbances or potential merger activity within the system. Color gradients indicate a central bulge region with older stellar populations giving off a redder/yellower light, surrounded by bluer regions possibly indicative of ongoing star formation. The central regions of the galaxy appear much more concentrated and dense when compared to the outer regions. Overall, the galaxy seems to be a dynamically evolving system with ongoing star formation, a non-spherical shape, and hints of interaction.
