The galaxy presents a generally smooth appearance, exhibiting an elliptical morphology. Its central region displays a bright, concentrated core, indicative of a high stellar density, likely with an older stellar population. The galaxy appears to be relatively symmetric and shows an intermediate ellipticity, neither perfectly spherical nor highly elongated. No distinct spiral arms or bar structures are discernible. Faint color gradients may indicate differences in stellar populations throughout the galaxy, with bluer hues potentially present in the outer regions suggesting the presence of younger stars or ongoing star formation, but these are subtle. There is no visual evidence of significant tidal disturbances, major mergers, or strong interactions with other galaxies. Any ongoing star formation is likely occurring at a low rate.
