The galaxy presents an elongated morphology, indicative of a likely disk-shaped system viewed at an oblique angle. A prominent central bulge appears to be the dominant feature, exhibiting a yellowish hue that suggests an older stellar population. Fainter, bluish regions are observed extending from the central bulge, possibly indicating areas of more recent star formation within the galactic disk. The disk appears slightly disturbed, suggesting the possibility of an ongoing interaction or past merger event, although a clear companion galaxy is not evident in the immediate vicinity. The galaxy's overall color gradient, shifting from yellow in the center to blue toward the outer regions, is consistent with a galaxy that has experienced some degree of ongoing or recent star formation activity.
