The galaxy presents a distinct spiral morphology. It is viewed at an oblique angle, but not perfectly edge-on. Two prominent spiral arms are discernible, winding loosely around the galactic center. These arms exhibit a patchy, somewhat diffuse structure, hinting at regions of active star formation. The central bulge appears moderately sized and exhibits a yellowish hue, suggesting an older stellar population. A subtle bar feature seems to traverse the central region, elongated along the major axis of the galaxy. Overall, the galaxy does not appear to be undergoing any major merging activity, though there is some indication of minor disturbances within the disk. The color profile indicates a mix of stellar populations, with bluer tones apparent in the spiral arms and redder tones concentrated towards the bulge.
