The galaxy presents as a relatively smooth, centralized object. It appears elliptical in shape, showing a slight elongation. The core is a bright yellow-white, indicating older stellar populations. Surrounding the core is a more diffuse halo with a greenish tint, suggesting the presence of some younger, hotter stars, or potentially emission from ionized gas. The overall structure lacks any clear spiral arm features or significant dust lanes. There is no obvious evidence of a major ongoing merger or significant tidal disturbances. The galaxy appears to be relatively isolated and undisturbed.
