The observed galaxy exhibits a complex morphology, suggestive of an ongoing or recent interaction. It appears as a relatively bright object with a diffuse central region. The galaxy's overall shape is somewhat elongated, deviating from a perfect spheroid. Evidence of disturbance is visible, with possible tidal features or asymmetries indicating gravitational interaction with another galaxy, even if it is not immediately apparent within the image. The color profile suggests a moderately evolved stellar population.
