The galaxy presents as a predominantly smooth, elliptical structure, exhibiting a concentrated central bulge. The color profile suggests a higher concentration of older stellar populations, with a notable lack of blue color indicative of recent star formation. There is no obvious spiral arm structure or significant dust lane features visible. The isophotes appear relatively regular and undisturbed, with no signs of major mergers or tidal disruptions. The galaxy is slightly elliptical, appearing quite round, with a suggestion of minor asymmetry in its outer regions, although this could be due to image artifacts. The object displays a consistent color gradient from the center outwards, which is expected from elliptical galaxies. Overall, the galaxy appears as an evolved system with a significant stellar mass and a quiescent star formation history.
