The galaxy presents as a spiral structure, though disturbed. A prominent central bulge exhibits a yellowish hue, likely indicating an older stellar population. Emanating from the central bulge are somewhat irregular and flocculent spiral arms. The arms show signs of both blue and green colors, suggesting a mix of ongoing star formation within regions of ionized gas. The disk is not perfectly face-on, with an inclination that allows partial viewing of the galaxy's structure. There appears to be evidence of interaction or a possible merger event in its morphology. There is some amorphous structure adjacent to the galaxy, and it is quite perturbed, hinting at possible merging event in the past or present. Overall, the galaxy seems to be undergoing some type of transformation.
