The galaxy presents a complex morphology, appearing to be a likely interacting system. A prominent, relatively smooth, and concentrated central bulge or core region dominates the upper portion of the galaxy's profile, exhibiting a yellowish-orange hue indicative of an older stellar population. Below this central region, a fainter, more diffuse area with hints of blueish color suggests the presence of younger stars and possible ongoing star formation. This lower region may represent a disturbed or distorted disk component. Evidence for interaction can be seen in the asymmetry and disrupted appearance of the fainter disk-like structure. There may be tidal tails or bridges of material, although indistinct. The galaxy's low specific star formation rate suggests that star formation has largely ceased or is occurring at a very low rate, with the dominant light coming from older stars in the central bulge. Overall, it appears to be a galaxy undergoing or having recently undergone a significant gravitational interaction.
