The galaxy appears to be a spiral galaxy viewed nearly edge-on. A prominent dust lane bisects the central bulge, obscuring the light from behind it. The bulge itself is bright and concentrated, with a slight yellowish hue that may indicate an older stellar population. Fainter, reddish regions are observed in the disk, suggestive of ongoing star formation. The overall morphology is consistent with a disk galaxy exhibiting some level of internal disturbance, although a full merger cannot be ruled out, it appears undisturbed. The color gradient from the bulge to the outer disk suggests variations in stellar populations and dust content.
