The galaxy presents a somewhat elliptical morphology, though with hints of a possible disk structure. The central region exhibits a high degree of luminosity, suggesting a concentration of stars or an active galactic nucleus. There appears to be a color gradient from the center outwards, with the core being a brighter white, possibly indicating older stars or dust obscuration.

The outer regions are less well-defined, blurring out, with a fainter, bluer halo possibly indicative of younger stellar populations or ongoing star formation, although the rate seems relatively low. There are no immediately obvious signs of major mergers or tidal disturbances, but there may be some minor irregularities in the outer halo that warrant further investigation. Overall, the galaxy appears relatively smooth in structure.
