The galaxy presents as a roughly elliptical form, exhibiting a central bulge that is somewhat bright. Evident are signs of disturbance in its morphology, hinting at possible gravitational interactions. A faint tidal tail or stream of stars and gas extends from the main body, suggesting a past or ongoing merger event. There may be a second, smaller galactic object also visible that appears to be a different color from the main galaxy. The outer regions display some structural complexity and potentially a disk component, though these features are not sharply defined. A fraction of the light from the galaxy is visible in the blue part of the spectrum, which would suggest active star formation. Some redder regions may signify older stellar populations. Overall, this galaxy exhibits signs of dynamic activity.