The galaxy presents an elongated, cigar-shaped morphology, viewed at a high inclination. The central bulge region exhibits a predominantly yellowish-orange hue, suggestive of an older stellar population. Fainter, greenish diffuse patches extend along the major axis of the galaxy, hinting at regions of potential star formation. There is a possible slight irregularity in the disk on the lower side of the image, which may indicate a minor gravitational disturbance, but it could also be the result of image noise. Overall, the galaxy appears to be relatively smooth in its structure with little sign of major mergers or interactions.
