The observed galaxy presents an elliptical morphology, appearing as a flattened disk when viewed from our vantage point. The central region exhibits a significant concentration of light, suggesting a prominent galactic bulge or core. The light appears to be a more intense and potentially of a different stellar population than that of the galactic plane. The outer regions of the galaxy show evidence of disk-like structure, with a more diffuse and less concentrated luminosity profile. There are hints of spiral arm structure, though it appears quite faint and could be described as being a galaxy with a possible distorted disk due to merging. Although the disk is somewhat smooth, it may be undergoing a minor disturbance such as a merger.
