The galaxy presents a generally smooth and concentrated morphology. It appears elliptical or lenticular in shape, exhibiting a high degree of radial symmetry. The central region displays a bright, yellowish core, indicative of an older stellar population and a likely concentration of mass. Fainter, more diffuse material extends outwards from this central region, forming a halo of diminishing intensity. There is a slight color gradient, with the central region appearing more yellow and the outer regions tending toward a blue/green hue. No distinct spiral arms or bar structures are evident. The overall impression is one of a mature galaxy with little evidence of recent major mergers or significant ongoing star formation, although some low-level activity cannot be ruled out based on the color and shape of the galaxy alone. Small disturbances or tidal tails are not visible.
