The galaxy presents as a fairly smooth, elliptical-type object, exhibiting a high degree of central concentration. The light profile appears relatively uniform, transitioning smoothly from a bright, unresolved core to a fainter, extended halo. There is no obvious dust lane, spiral arm structure, or any sign of recent major merger activity. The color appears to be generally consistent, with a slight reddening toward the core, possibly indicating an older stellar population in the central regions. There appears to be no substantial star formation visible. Overall, the galaxy appears to be a relatively quiescent system.
