The galaxy presents as a spiral type, exhibiting a prominent disk structure. Evident spiral arms extend from a central bulge, although their morphology appears somewhat disturbed. The color distribution across the galaxy is heterogeneous. The central bulge exhibits a yellowish hue, suggesting an older stellar population. The spiral arms display a bluer tint, indicative of ongoing star formation, with the presence of reddish regions potentially signifying areas of intense star formation or dust obscuration. The overall form is suggestive of a recent or ongoing interaction or merger event, as the spiral structure is not entirely well-defined and shows asymmetry.
