The galaxy presents a distinct morphology suggestive of a spiral galaxy viewed at a relatively high inclination. A prominent central bulge exhibits a yellowish-orange hue, indicating an older stellar population. Extending from the bulge, a fainter, elongated disk structure is visible. This disk appears less structured and somewhat diffuse, with a bluer color gradient compared to the bulge, potentially indicating ongoing or recent star formation. The overall light distribution suggests a moderate degree of smoothness, although some irregularities within the disk region may hint at internal processes such as minor gravitational disturbances. Based on the apparent lack of significant tidal features or close companions, it is likely not undergoing a major merger event. The color profile, while not explicitly segmented into prominent spiral arms, does indicate regions of differing stellar populations within the disk.
