The galaxy presents as a spiral type, with a moderately sized bulge. Distinct spiral arms are visible, wound relatively tightly around the central bulge. There appear to be two main spiral arms, with some branching. The arms display a bluer color indicative of younger star populations, while the bulge exhibits a yellow-white hue, possibly indicating an older stellar population. A subtle bar structure appears to be present within the inner region of the galaxy. Indications of minor disturbances or interactions are also observed, potentially suggesting a past or ongoing minor merging event.
