This galaxy, observed at a redshift of approximately 0.3, exhibits a complex morphology suggesting ongoing or recent interaction. The light distribution is dominated by a relatively smooth, centrally concentrated component with a yellow-red hue, indicative of an older stellar population. This component appears moderately round, but not perfectly spherical.

A distinct, irregularly shaped region of bluer light is observed extending from the main body of the galaxy, indicating active star formation. This blue region suggests the presence of younger, hotter stars.

The overall light profile suggests a transition stage galaxy. It has characteristics somewhere between an elliptical galaxy and a spiral galaxy, but also shows evidence of disturbance from a merger. There is also some minor evidence of asymmetry, which may arise from tidal effects from the merger.
