This galaxy presents as an edge-on spiral or lenticular galaxy with a distinct bulge. The bulge exhibits a yellowish-orange hue, suggestive of an older stellar population. The galactic disk appears relatively thin and elongated. Faint blueish halos extend outward from the main disk, possibly indicating regions of more recent star formation activity. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or significant tidal distortions. A slight asymmetry in the disk is observable, but not enough to indicate a major ongoing interaction. There may be a hint of a boxy bulge structure, but the resolution is low. Dust lanes within the disk are not readily apparent from this observation.
