The galaxy presents as a somewhat amorphous, irregular structure with diffuse boundaries. Its overall shape appears elongated, deviating from a perfect elliptical or spiral form. The core region exhibits a brighter, more concentrated luminosity, indicative of a higher density of stars or active galactic nucleus activity.

Distinct regions of intense star formation are suggested by the presence of blue-shifted light, particularly in the outer parts of the galaxy. The redder hues scattered throughout indicate older stellar populations or dust obscuration. The galaxy shows hints of disturbance, possibly related to interactions with another galaxy, with potential tidal tail formation or other asymmetry. There is no clear presence of spiral arm structures, bar or disk and might be undergoing a merger or strong starburst event.
