The galaxy presents a largely smooth, elliptical morphology, lacking prominent spiral arms or a well-defined disk structure. A concentrated central bulge is visible, exhibiting a yellowish hue, suggesting a population of older stars. The outer regions display a subtle color gradient, transitioning to a slightly bluer shade, potentially indicative of more recent, albeit subdued, star formation activity. The galaxy appears relatively isolated with no signs of major mergers or tidal disturbances; small irregularities may or may not indicate a minor interaction. The overall rounded shape and smooth appearance suggest that this galaxy is a relatively relaxed system.
