The galaxy appears as a moderately bright, somewhat diffuse object. Its shape is generally elliptical, with a suggestion of a slight elongation, but it is primarily rounded. The light distribution is concentrated towards the center, displaying a notable bulge. There's a gradual decrease in luminosity extending outwards from the core, indicating a smooth decline in stellar density. 

There are faint, diffuse features at the edges of the galaxy's light distribution. These are potentially faint spiral arms or tidal features resulting from gravitational interactions. No obvious dust lanes or distinct spiral structures are visible. The color gradient transitions from a yellow-orange at the core to a blue-green tint in the outer regions. This might suggest older stellar populations are in the center, and a possible lower amount of ongoing star formation there. The outer regions may contain younger, bluer stars. There may be some mild gravitational disturbance.
