The galaxy presents as a spiral galaxy viewed at an oblique angle. A prominent central bulge dominates the core region, exhibiting a yellow-white hue indicative of an older stellar population. Spiral arms are clearly visible extending from the central bulge. These arms display a bluer color, implying the presence of younger, hotter stars and active star formation regions. The spiral arms exhibit a relatively well-defined, two-armed structure, with a medium winding. There appears to be a bar-like structure extending through the bulge. There is no evidence of a major merger event. The outer disk shows hints of possible dust lanes. The galaxy appears to be experiencing star formation at a modest rate.
