This galaxy appears to be a late-type spiral, likely viewed edge-on. The disk is prominent, with a slight bulge that appears predominantly rounded. The galaxy displays no obvious major or minor disturbances suggestive of recent or ongoing major mergers. No distinct dust lanes are visible. The galaxy’s color indices suggest a moderate degree of ongoing star formation, with a stellar mass perhaps on the higher end. Its specific star formation rate is likely relatively low. The light distribution indicates that it likely has structural features or disk morphology.