The galaxy presents as an elongated structure, with an aspect ratio indicating a cigar-like shape. The central region exhibits a concentrated luminosity, suggesting the presence of a bulge or a high density of stars. This central bulge is noticeably yellow/orange in color. As we extend outwards from the center, there is evidence of a disk-like structure. On one side of the core the color is still somewhat yellow, but less bright, while on the other side, it changes to a blueish hue. This region might suggest on-going star formation. There are no strong indicators of spiral arms from what is visible, and no obvious signs of a major ongoing merger event. The galaxy could be undergoing a minor interaction or exhibit internal disturbances.
