The galaxy appears to be a relatively smooth, elongated structure. Its morphology is suggestive of an edge-on spiral or a lenticular galaxy, with a noticeable bulge that gradually fades into a disk. There may be a disk, though it is challenging to discern substructure or spiral arms with the available resolution. The color profile indicates a redder hue in the central region, possibly denoting an older stellar population, while the edges appear slightly bluer, potentially indicating younger stars. The galaxy displays little sign of significant disturbances or ongoing major mergers.
