The galaxy exhibits a disk-like morphology with a central bulge. The bulge appears relatively prominent and displays a yellowish-orange hue, possibly indicating an older stellar population. The disk component shows a bluer tint, suggestive of ongoing star formation. Some irregular features are present within the disk, potentially indicating spiral arm structure or signs of a minor disturbance. Overall, the galaxy appears moderately inclined with respect to our line of sight. Its estimated size is a few kiloparsecs across. There are no clear signs of a major merger event.
