This galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. The overall shape is elongated, tending toward a cigar shape, with an apparent lack of defined spiral arms or a distinct disk structure. It appears undisturbed, without any obvious signs of ongoing mergers or major interactions. There is a slightly blueish hue to the central region, which may indicate some recent star formation activity, although the galaxy is primarily composed of older stellar populations. The light distribution fades gradually from the center outwards.
