The galaxy presents a predominantly elliptical morphology, appearing largely smooth and well-rounded. Its color profile indicates a higher concentration of older stellar populations, with the central region exhibiting a yellowish hue. The galaxy lacks any distinct spiral arm structures or prominent dust lanes, suggesting a more quiescent star formation history. There's a subtle color gradient from the central bulge outwards, with the outer regions showing a slightly bluer tint, hinting at the presence of younger stars, though less substantial. The overall light distribution is centrally concentrated, indicating a significant bulge component, consistent with an early-type galaxy classification. There is no evidence of active galactic nuclei or strong tidal interactions.
