The galaxy presents a flattened elliptical morphology, displaying a smooth, featureless appearance across its visible structure. A concentrated, bright central bulge dominates the galaxy's core, exhibiting a yellowish hue suggestive of an older stellar population. Moving outward from the core, the luminosity gradually decreases into a more diffuse halo. This halo appears less yellow, with a hint of bluer tones, which could indicate some ongoing, but low-level, star formation activity. There is a slight asymmetry visible in the outer regions, possibly indicative of a minor gravitational interaction or past merger event, however the main galaxy does not show strong merging characteristics. The overall structure suggests a galaxy that is relatively evolved, transitioning away from active star formation in the main body.
