The galaxy presents as a relatively smooth, centrally concentrated object, with a somewhat elliptical shape. The central region appears brighter and more uniform, suggesting the presence of a bulge possibly populated with older stars. There is evidence of a faint, disk-like structure surrounding the bulge, exhibiting a subtle blueish tint, which may indicate ongoing or recent star formation. The galaxy does not show any obvious signs of strong disturbances or major merging events, but there may be minor asymmetries present in the outer regions. The overall morphology suggests a galaxy somewhere between a pure elliptical and a spiral, possibly an early-type spiral or lenticular galaxy seen at a considerable distance.
