The galaxy presents a somewhat amorphous shape, with a suggestion of a disk-like structure viewed at an oblique angle. The central region appears more concentrated and exhibits a slightly redder hue, possibly indicating an older stellar population or higher dust content. Extending outwards from the center are diffuse, bluer regions, suggestive of younger star formation. There are hints of faint, irregular extensions or tidal features. These features may indicate past or ongoing interactions with other galaxies, although there is no clear evidence of a major merger. The galaxy exhibits a mixture of smooth light distribution and areas with more irregular texture.
