The galaxy presents an overall elliptical morphology, appearing somewhat elongated, cigar-shaped. A dominant, smoothly distributed light component is observed, concentrated toward the center, suggesting a significant bulge.

A faint, disk-like feature extends from the central bulge. Hints of spiral arms can be seen, but are not well-defined. One arm is much more pronounced than the other, and it appears that the larger arm is being warped or disturbed.

The galaxy exhibits a color gradient, with the central region appearing more yellow/red, and the outer regions appearing more blue/white. This may indicate that the bulge is primarily composed of older stars, whereas the disk contains a population of younger, hotter stars undergoing active star formation. Evidence of a minor interaction is possible in the warped disk.
