The galaxy presents as a disk-shaped structure, viewed at an oblique angle, with its major axis oriented roughly horizontally in the frame. It displays prominent spiral arms that emanate from a brighter, more concentrated central bulge. The bulge exhibits a yellowish hue, suggesting a population of older stars. The spiral arms, in contrast, show a bluer color, indicative of ongoing star formation and the presence of younger, hotter stars. There is no visual evidence of a strong central bar. The arms appear somewhat tightly wound, contributing to an overall ordered spiral morphology. A slight asymmetry or disturbance may be present, with the spiral structure appearing less defined on one side of the galaxy than the other, possibly indicating a past or ongoing interaction with another galaxy. The disk appears elongated, with an estimated ratio of minor to major axis of approximately 0.4. Overall, the galaxy exhibits characteristics of a spiral galaxy with a dominant disk component and evidence of both older stellar populations in the bulge and active star formation in the spiral arms.
