The galaxy appears as a relatively smooth, though not perfectly spherical, object. It exhibits a centrally concentrated brightness profile, suggesting a significant bulge component. The overall color is somewhat red, possibly indicating an older stellar population and/or a degree of dust obscuration. There is only the slightest hint of spiral arm structure, if any. The galaxy appears relatively isolated with, at most, a minor companion or tidal feature possibly indicating a past or ongoing minor interaction. The image does not reveal any strong signs of active galactic nucleus activity.
