This galaxy presents a complex morphology. The primary body of the galaxy is a somewhat elliptical, though not perfectly smooth, structure. A central bulge is discernible, appearing more concentrated and exhibiting a yellowish hue, suggesting an older stellar population. Extending outward from this central region, we observe fainter, more diffuse regions that appear less symmetrical, hinting at possible disturbances. To one side of the main galactic body, a fainter region shows hints of a spiral arm structure.

The overall color profile indicates a mix of stellar populations. The yellowish central bulge suggests a population of older, redder stars, while the bluer tinges in the outer regions may indicate the presence of younger, hotter stars, and regions of star formation. There's evidence of a non-negligible rate of star formation occurring within this galaxy. Based on the asymmetry of its shape and possible distortions, it appears this system may be undergoing a minor interaction with a smaller system.
