The galaxy appears to be a relatively compact object, presenting a smooth, somewhat elliptical morphology, although some features are present. The light distribution is centrally concentrated. The object appears to be transitioning between spheroidal and disk-like in shape. There is a slight hint of asymmetry, possibly indicating a minor interaction or disturbance. There is some evidence of internal structure, hinting at a possible disk component. Overall, the galaxy seems to be an intermediate mass system with a low current star formation rate. There is no clear sign of a major merger, however, the galaxy is not perfectly undisturbed.
