The galaxy presents as a spiral, viewed at an oblique angle. A prominent central bulge dominates the core region, which appears nearly spheroidal and displays a smooth, yellowish hue. The spiral arms extending from the central bulge are somewhat tightly wound. These arms exhibit a mottled appearance with regions of blueish color, suggestive of ongoing star formation. There is no obvious bar structure visible in the image. The outer disk appears to be relatively smooth, although fainter and less defined, suggesting an older stellar population compared to the spiral arms. There is little evidence of significant morphological disturbances or tidal features, implying a relatively quiescent merger history.
