The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, which appears to be the brightest region. Moving outwards from the bulge, the light gradually fades, suggesting a decrease in stellar density and/or younger stellar populations. There is little indication of spiral arm structure or significant dust lanes. The overall color appears to be yellowish-white, indicative of an older stellar population, but there appears to be some bluer light in the outskirts of the galaxy, suggestive of the presence of some ongoing, but low level, star formation. The shape is roughly rounded. There is no clear evidence of any major ongoing merger activity. The overall structure is largely undisturbed, lacking significant tidal tails or distortions.
