The galaxy presents a disturbed morphology, appearing as a relatively compact object with a diffuse halo. There are indications of tidal features, possibly faint streams or shells, suggesting an interaction or merger event in its recent history. Color gradients within the galaxy are subtle, but suggest the presence of both older stellar populations and regions of ongoing or recent star formation. The object does not appear to have a clearly defined spiral structure or a dominant bulge. There appears to be a relatively luminous core region, though the overall light distribution is not perfectly smooth. There is some hint of dust lanes or obscuration in the inner regions. Based on the overall appearance, the galaxy appears to be an interacting or post-merger system.
