The galaxy presents as a disk galaxy, observed at an oblique angle relative to our line of sight. The central region exhibits a bright, concentrated bulge component which appears yellowish in color. The disk structure surrounding the bulge shows a mottled texture, likely indicating regions of star formation. While spiral arm features are not sharply defined, the distribution of light within the disk suggests the possible presence of loosely wound arms. The outer regions of the disk fade gradually into the background, indicating a decreasing stellar density. The galaxy appears relatively isolated, with no obvious signs of major tidal disturbances or ongoing mergers. The overall shape is elliptical, indicating that it's not perfectly face-on to us.
