The galaxy presents an elongated, disk-like morphology, viewed at a moderately oblique angle relative to our line of sight. A prominent central bulge is evident, characterized by a bright, concentrated luminosity with a yellow hue, suggestive of an older stellar population.

Surrounding the bulge, a disk structure extends outwards. The disk exhibits a mottled texture with a mix of light and dark regions. Some areas of the disk display a slightly bluer tinge compared to the bulge, indicating the presence of younger, hotter stars. Patches of dust are suspected within the disk, contributing to the observed irregular light distribution and potentially obscuring background stars or gas clouds.

There is some evidence of minor distortions within the outer regions of the disk, such as subtle asymmetries or faint plume-like extensions. These features might be indicative of past minor interactions or disturbances. The overall structure suggests a spiral or lenticular galaxy type, though without higher resolution, a definitive classification is difficult.
