This galaxy exhibits a disk-like morphology with a central bulge. The disk component appears to be viewed at an angle, possibly close to edge-on, which obscures a full face-on view. There appears to be some disturbance in the disk, possibly indicative of a minor interaction or internal dynamical processes. Star formation appears to be occurring, as evidenced by the presence of bluer regions, particularly at the edges of the visible disk. The bulge presents a smoother, more uniform color profile, indicating a population of older stars with less recent star formation. The galaxy does not display strong signs of a major merger event, though minor irregularities are present.
