The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated central bulge that gradually fades into a more diffuse halo. The overall shape is generally round, with only a slight deviation from perfect circularity. There is no apparent spiral arm structure or strong evidence of a disk component. There's a hint of blueish color around the outer edges, indicating potential areas of recent star formation, though the overall color profile leans towards redder hues, suggesting a population dominated by older stars. There are no obvious signs of ongoing major mergers or tidal disturbances impacting the galaxy's structure.
