The galaxy presents as a luminous object with a central bulge, elongated along its major axis. The color profile indicates a dominant yellow-red hue within the core, suggesting an older stellar population. Fainter, diffuse blue light is observed in the surrounding area, possibly due to the presence of younger stars. There appears to be a disk, but it seems highly disordered. The overall structure suggests an intermediate morphological type, somewhere between an elliptical and a spiral. There is a possibility of interaction with a smaller, more distant galaxy nearby.
