The galaxy appears as an elliptical or lenticular structure, exhibiting a relatively smooth morphology. The central region displays a yellowish hue, potentially indicative of an older stellar population. Moving outward, the color transitions to a bluer shade. There appears to be some evidence of a disk-like structure present as well as some features that imply the galaxy may be slightly disturbed. I estimate that the rate of forming stars is slow. It does not appear to be undergoing a major merger.
