The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a bright, yellowish-white hue, suggesting a high density of older stars. Moving outward from the center, the galaxy fades gradually into a less distinct halo. Faint, diffuse blue tinges appear within the halo surrounding the central bulge and within the outer regions, which may indicate areas of more recent or ongoing star formation. There are no prominent spiral arms, bars, or significant dust lanes visible. Subtle irregularities or minor disturbances are not apparent in the overall structure. The galaxy does not appear to be undergoing any major merging events, but subtle disturbances cannot be ruled out due to the faintness of the halo region. It appears the galaxy is relatively isolated.
