The galaxy appears as a relatively compact object with a bright, centrally concentrated core. The core exhibits a predominantly cyan hue, suggestive of significant emission in the blue and green portions of the visible spectrum, potentially indicative of active star formation or an active galactic nucleus. The galaxy lacks a clearly defined spiral arm structure or a smooth, elliptical morphology. The overall shape is somewhat irregular, with subtle protrusions or asymmetries extending from the central region. There is evidence of a diffuse, fainter halo or envelope surrounding the bright core. Close inspection reveals hints of minor disturbances in the outer regions, possibly due to a past merger event or interaction with a smaller companion galaxy. Overall, the galaxy presents a complex morphology characterized by a bright core, irregular shape, and subtle signs of past gravitational interactions.
