The galaxy presents a generally smooth, elliptical morphology. The central region is characterized by a bright, concentrated core, suggesting a high stellar density and potentially the presence of an active galactic nucleus or a supermassive black hole. The galaxy exhibits a radial color gradient, with the core appearing more yellow/white and the outer regions displaying a bluer hue. This color difference might indicate varying stellar populations, with older, redder stars concentrated in the core and younger, bluer stars in the outer regions.

There is no clear evidence of distinct spiral arms or a well-defined disk structure. However, some subtle irregularities in the outer regions might suggest minor tidal disturbances, potentially due to past interactions with smaller galaxies. The overall structure appears relatively undisturbed, with a high degree of central concentration and little indication of ongoing major mergers. The galaxy exhibits a moderate level of star formation. The galaxy is generally round in shape.
