The galaxy presents as a relatively compact object. Its overall morphology appears to be neither purely elliptical nor a well-defined spiral. The light distribution suggests a structure that is somewhat disturbed. There is evidence of a central concentration of light, possibly indicative of a bulge or nucleus. Extending outward from this central region, there is an area of diffuse light. The shape of this is elongated and possibly a tidal tail. One section is blue, another is redder, and there appears to be a bridge that connects the two sections. There may be evidence of ongoing or past interactions, suggesting a potential merger event or tidal disruption.
