This galaxy presents as a relatively smooth, disk-shaped system. The central region exhibits a concentrated, bright, yellowish hue, suggestive of an older stellar population. The outer disk appears somewhat elongated. There is a subtle bluer tint in the outer regions of the galaxy, which could indicate more recent or ongoing star formation, though it is quite subdued. While the primary structure is undisturbed, a possible minor tidal feature is faintly observed on one side, possibly indicating a minor interaction. Based on the apparent smoothness and color distribution, the system is likely a galaxy with a significant spheroidal component and a relatively quiescent star formation rate.
