The galaxy appears to be a spiral type, with a distinct disk structure. Two prominent spiral arms are visible, tightly wound around the central bulge. The bulge appears moderate in size, contributing significantly to the galaxy's overall luminosity. The colour gradient transitions from a yellowish hue at the core, likely indicative of an older stellar population, to bluer tones in the outer spiral arms, suggesting ongoing star formation. Patches of brighter regions are observable along the spiral arms, potentially signifying areas of enhanced star birth. The galaxy shows signs of minor disturbances in its morphology, and appears to be interacting with a smaller galaxy next to it.
