The galaxy presents a generally smooth, elliptical appearance. There is a centrally concentrated bulge that is largely homogenous in color, displaying a bright, slightly blue-white hue indicative of a population of younger stars. This bulge smoothly fades into a less defined, fainter halo region. There are no strong indicators of spiral arm structures. The overall shape is somewhat ellipsoidal, leaning towards roundness, with only the slightest indication of a cigar shape. There is no clear evidence of ongoing major mergers or significant tidal disturbances. A very slight hint of a minor interaction or disturbance might be present based on subtle asymmetries in the outer halo, however no significant merger can be observed.
