The galaxy appears to be a relatively smooth, elliptical system with a concentrated central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population with lower rates of recent star formation. The outer regions of the galaxy seem to fade gradually into the background, lacking distinct spiral arms or prominent features. There is some slight asymmetry and potentially a small amount of tidal disturbance, possibly indicating a past or ongoing minor interaction. Overall, the galaxy presents a spheroidal morphology, and there is a hint of a disk.
