The galaxy presents as a somewhat diffuse, yellowish-orange structure, indicative of an older stellar population and reduced ongoing star formation. It appears to be relatively large. There are hints of some type of disruption present, possibly a merger or tidal interaction. A fainter, more compact, bluish object is located adjacent to the main body of the galaxy, potentially indicative of a tidal dwarf galaxy or a smaller galaxy involved in an ongoing merger. Overall, the galaxy morphology suggests it is in a late stage of its evolution or is undergoing significant gravitational interaction. The light distribution is relatively smooth, but there are hints of some irregular features.
