The galaxy presents a generally smooth and somewhat amorphous morphology. There is evidence of a central bulge, possibly containing an active galactic nucleus. There appears to be a disk-like structure exhibiting some signs of disruption. Hints of what could be spiral arm fragments are present, but the overall form lacks well-defined spiral structure. A significant, luminous area is seen offset from the central core, suggesting either an ongoing merger event or a region of intense star formation. Colors are somewhat muted, with hints of blue indicating the presence of young, hot stars, but the overall color profile suggests a relatively passive star-forming environment. The galaxy's relatively compact size suggests it may be an elliptical or lenticular galaxy undergoing a disturbance. Faint tidal features indicate the possibility of past interactions with another galaxy.
