The galaxy presents as a somewhat amorphous structure, exhibiting a non-uniform light distribution. The central region appears relatively bright and concentrated, displaying a yellowish hue. This might indicate an older stellar population or significant dust obscuration in the core. Surrounding the central region, there is a more diffuse, fainter halo extending outwards. The color in this outer region shifts towards a bluer tone, potentially indicative of younger stars and ongoing star formation. There are indications of asymmetry and possible tidal features or disturbances. These features suggest that the galaxy may be undergoing or have recently experienced a merger event or gravitational interaction. Overall the galaxy lacks a defined spiral structure and appears to be somewhere between a classic elliptical and a disturbed spiral galaxy.
