The galaxy appears to be a spiral galaxy with a prominent, bright central bulge. The bulge is roughly circular and exhibits a yellowish hue, suggesting a population of older, redder stars. Fainter, bluer spiral arms extend outwards from the bulge, though they are somewhat indistinct and lack strong definition. The arms appear patchy and flocculent, with hints of star formation regions visible as slightly bluer knots. Overall, the galaxy presents a moderately smooth appearance, with some evidence of a disk-like structure, but no significant merging events or major disturbances are immediately apparent. It has an estimated redshift of 0.07, placing it at a cosmologically significant distance.
