The galaxy presents as a somewhat elongated, cigar-shaped morphology. The central region appears smooth and concentrated, displaying a yellowish-orange hue, which may indicate an older stellar population. Diffuse light extends from the center, forming a flattened disk-like structure oriented edge-on relative to our line of sight. There are subtle irregularities or minor disturbances visible along the edges of the disk, suggesting potential tidal interactions or ongoing accretion events. There seems to be a possible bulge at the center. Overall, the galaxy exhibits characteristics consistent with an early-type spiral galaxy, possibly undergoing morphological transformation.
