The galaxy presents as a somewhat elongated, lenticular or possibly spiral system viewed at an oblique angle. It exhibits a primarily smooth morphology, with a relatively high concentration of light towards the central region, indicating a prominent bulge. Faint spiral arms are either absent or very tightly wound, contributing to its overall smooth appearance. The bulge and the disk show a slight color gradient, transitioning from a more yellowish core to a bluer disk, suggesting ongoing star formation in the outer regions. The object exhibits some degree of asymmetry and potential minor tidal disturbances, hinting at past or ongoing interactions with nearby galaxies. The galaxy appears relatively isolated, with no immediately obvious major merging events occurring.
