The galaxy presents a generally smooth, elliptical morphology with a highly concentrated central bulge exhibiting a bright yellow-white hue, suggesting an older stellar population. There appears to be little to no evidence of a distinct disk structure. There is an extremely faint, diffuse halo surrounding the central region with only a slight blue tint, indicating a reduced rate of ongoing star formation in the outer regions. The overall shape appears nearly circular, showing no significant elongation. No signs of major mergers or significant tidal disturbances are evident within the immediate vicinity of the galaxy, although there is a hint of possible minor disturbance located off-center to the right.
