The galaxy appears as a flattened, elliptical-like structure with a smooth and centrally concentrated luminosity profile. The central region exhibits a brighter, yellowish hue, which could indicate an older stellar population dominating the core. This central region gradually fades into a more diffuse outer region with a reddish tint, suggesting the presence of dust or a slightly younger stellar population further away from the core. Faint, diffuse extensions are barely visible at each end of the galaxy, possibly indicating a weak disk structure. There's no apparent evidence of strong spiral arms or significant star formation regions within this galaxy. The overall morphology suggests a relatively evolved galaxy with a moderate mass and low star formation rate. Any disturbances or mergers appear to be minimal to non-existent based on the current visual data.
