The galaxy presents as a somewhat elongated structure. The central region exhibits a higher surface brightness, indicating a concentration of stellar mass and/or active galactic nucleus activity. Moving outwards from the center, the light becomes more diffuse. There appears to be a faint extension or possible tidal feature extending from the main body of the galaxy which could indicate a past or ongoing interaction with another galaxy, although it is not exhibiting any major disturbance. The color is relatively uniform across the galaxy, but there is a slightly bluer tint around the edge. This could mean that the star formation rate is relatively low throughout the galaxy, with a minor amount of newer stars around the edge. Overall, the galaxy appears relatively smooth, but with some irregularities in its shape.
