The galaxy presents as a somewhat elongated, disk-like structure seen nearly edge-on. The central bulge appears prominent and exhibits a yellowish-orange hue, suggestive of an older stellar population. The disk component displays a bluer tint, hinting at ongoing star formation, although the resolution limits detailed analysis of individual star-forming regions. The galaxy's overall morphology appears relatively undisturbed, lacking obvious signs of major mergers, though there is a hint of slight asymmetry in the outer regions of the disk, potentially indicating minor gravitational interactions. The overall smooth appearance suggests a galaxy that is either an elliptical or a spiral galaxy that is viewed edge-on.
