The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge exhibiting a yellowish-white hue. The outer regions show a subtle transition in color towards a bluer tint, although this is not strongly pronounced, suggesting a modest level of on-going star formation. There may be faint indications of subtle disturbances or asymmetry within the outer halo, potentially indicative of minor gravitational interactions, but this requires further investigation. The galaxy's overall form leans towards a rounded shape, lacking the distinct spiral arm structure typically observed in disk galaxies.
