The galaxy presents as an elongated, somewhat disturbed system. A dominant, central bulge or core region exhibits a bright, concentrated luminosity. The overall color of this central region appears slightly yellow to white, suggestive of an older stellar population.

Extending from the central region are faint, diffuse structures. The color of the light suggests ongoing, but not vigorous, star formation, particularly in one end that appears bright red. The relative intensity of the red light from the right end suggests that it's the part with the most active star formation.

The galaxy does not display a well-defined spiral arm structure, appearing relatively smooth overall. There is some indication of asymmetry in the distribution of light, which could be the result of past interactions or mergers. Overall, the object appears to be a relatively massive system undergoing active star formation.
