The galaxy presents as a relatively smooth, disk-shaped structure with an elliptical morphology. Its color profile suggests a mature stellar population, exhibiting a yellowish-orange hue, particularly concentrated towards the central bulge. This indicates a likely absence of significant ongoing star formation within the bulge. 

The outer regions of the disk exhibit a slightly bluer tint, potentially indicating the presence of younger stars or some residual star formation, although the overall smooth appearance suggests any such activity is not dominant. The lack of pronounced spiral arm structures or irregular features further points to a relatively undisturbed and evolved galaxy. There is a possible slight warp or asymmetry visible in the disk, although it is subtle, suggesting the possibility of a past minor interaction or disturbance. The galaxy does not appear to be undergoing a major merger event.
