The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light profile with a dominant bulge. The light is characterized by a yellowish-orange hue, suggesting an older stellar population with fewer young, hot stars. There is no apparent spiral structure or prominent dust lanes. It appears relatively isolated, with only a few nearby faint objects that may or may not be interacting with it. There is some minor asymmetry present. The central region of the galaxy shows a higher concentration of light, possibly indicating the presence of an active galactic nucleus or a dense stellar core. The outer regions gradually fade into the background sky, lacking a sharp defined edge. There is some evidence of possible tidal features or faint plumes extending outwards, potentially indicating past merger events or gravitational interactions.
