The galaxy appears as a centrally concentrated object with a largely smooth morphology. The core region exhibits a bright, high-surface-brightness profile, potentially indicative of a dense stellar population and/or an active galactic nucleus, although no distinct jet-like structures are apparent.

Moving outwards from the core, a slightly fainter, extended halo surrounds the central region. The overall shape of the galaxy appears largely elliptical with a high degree of roundness. There is faint evidence of asymmetry or tidal disturbances. Overall, the galaxy's light distribution is well behaved, with no obvious signs of major mergers or disruptive events. There are no apparent spiral arms. There are no very strong blue clusters, so it appears to be composed primarily of older star populations.
