This galaxy presents as an edge-on spiral, exhibiting a pronounced disk structure viewed nearly parallel to our line of sight. The central bulge is moderately bright, appearing somewhat elongated and with a slight boxy shape. A thin dust lane is visible along the galactic plane, obscuring some of the light from the bulge. There is evidence of ongoing star formation, primarily concentrated in the outer regions of the disk. A faint green emission is visible near the dust lane. No signs of major mergers or significant tidal disturbances are apparent. The overall color is indicative of a mix of stellar populations, with older stars dominating the bulge and younger, bluer stars tracing the spiral arms within the disk. The galaxy appears to be relatively isolated in its immediate environment.
