The galaxy exhibits a complex morphology. At its core, there is a bright, compact region of intense blue light, suggesting a high concentration of young, hot stars or potentially an active galactic nucleus. Emanating from this central region is a fainter, elongated structure extending outwards. This extension has a yellowish-orange hue, indicative of an older stellar population or significant dust obscuration. The shape of the galaxy does not conform to a typical elliptical or spiral structure, showing signs of possible tidal disruption or interaction with another galaxy. There is no obvious grand design such as spiral arms, with only minor visual disturbances. The galaxy appears relatively isolated.
