The galaxy presents with an overall elliptical morphology. There is a central, concentrated bulge region. This bulge exhibits a primarily red-shifted color profile, implying an older stellar population. Fainter arms or extensions emanate from the central bulge. There is an indication of blue shift in parts of the galaxy.

Based on visual assessment, the galaxy shows signs of interaction or a previous minor merger event. The structure is disturbed with diffuse emission in its outer regions. While there is not a clear disk structure, some features suggest the presence of a disrupted or incomplete disk component.
