The galaxy presents an overall smooth morphology with an estimated effective radius of approximately 7 kpc. The object appears yellowish-white in color, suggesting an older stellar population and relatively low levels of ongoing star formation. The galaxy exhibits a somewhat rounded appearance, but displays evidence of a potential merger or tidal disturbance. There is a complex central region with what appears to be merging bodies. This region is likely associated with ongoing tidal disruption or remnant of a recent major merger event.
