The galaxy presents as an edge-on disk galaxy with a prominent, relatively bright central bulge. The disk exhibits a smooth appearance, showing limited discernible spiral structure or distinct star-forming regions. The light distribution suggests the presence of an older stellar population dominating the bulge, with bluer hues observed in the disk potentially indicating more recent star formation, though this is less prominent. The disk appears thin and elongated, displaying a high degree of symmetry across its major axis. There is no clear evidence of significant tidal interactions or ongoing mergers.
