This galaxy exhibits a disk-like morphology, appearing somewhat elongated. The central region displays a bright, concentrated luminosity, suggesting a relatively dense stellar population, possibly a bulge. A faint, diffuse halo surrounds the central core. The galaxy shows signs of disturbance. There is a slight asymmetry visible, with a potential tidal feature or minor arm extending from one side. The color appears to be bluer in the outer regions and whiter near the center. There is another galaxy close by, so this galaxy may be interacting with it. The light profile appears to be smooth overall, but a small amount of clumpy structure may be present in the outer regions. This warrants further investigation.
