The galaxy exhibits a centrally concentrated morphology with a relatively small angular size. The core displays a bright, compact region, likely indicative of a dense stellar population or active galactic nucleus. The color profile suggests the presence of both older, redder stellar populations, and areas of ongoing star formation exhibiting bluer hues, possibly due to a difference in the distribution of gasses or dust. There is evidence of significant disturbance to the system. A single arm appears to extend from the galaxy, wrapping tightly around it. There are no clear indications of a strong tidal interaction or major merger event. The general appearance is consistent with an irregular morphology, possibly a result of a minor merger.
