The galaxy presents a generally smooth and elliptical morphology. There is a concentrated central bulge, appearing yellowish. The outer regions exhibit a faint, diffuse halo. The overall color index suggests a population dominated by older stars, with a moderate redshift. There is no clear evidence of spiral arms or significant dust lanes. The galaxy appears relatively isolated, without any obvious signs of major mergers or strong tidal disturbances, although there may be a subtle asymmetry in the outer halo, potentially indicating a minor interaction.
