The galaxy presents a generally smooth, elliptical morphology. There is a concentrated central bulge that appears roughly spherical, emitting primarily light in the yellow-orange part of the spectrum. A slightly fainter and bluer halo surrounds the bulge, extending outwards in a somewhat flattened distribution. There is no obvious spiral structure or bar visible; however, the color variation suggests some level of ongoing star formation. There is no strong evidence of tidal tails or other significant distortions that would indicate a recent major merger, although some minor disturbances cannot be ruled out. The shape appears generally round with only a slight elongation. Overall, the galaxy appears to be a relatively quiescent system.
