The galaxy presents as an edge-on spiral, exhibiting a notable disk structure. The bulge appears to be rounded and dominates the central region, showing a concentrated distribution of older stellar populations indicated by its yellowish hue. The disk is relatively smooth, with no visible prominent dust lanes or spiral arm features discernible in this image. The galaxy has a moderate size and is well-defined, with no indications of major merging activity or significant tidal disturbances. There is a slight asymmetry in the disk's outer regions, possibly indicating minor gravitational interactions or past accretion events.
