The galaxy presents a morphology that appears to be somewhere between smooth and possessing distinct features. A central, brighter region is visible, possibly indicating a bulge or concentrated nucleus. There is a slight asymmetry in the overall shape, suggestive of a possible disk component or past interaction. 

The galaxy exhibits a range of colors, with a yellowish core potentially indicative of an older stellar population, and hints of bluer regions, which could signify ongoing or recent star formation. The lack of distinct spiral arms suggests that if it is a spiral galaxy, it is not a well-defined one, or that it is being viewed at an angle that obscures the spiral structure.

There are some indications of potential tidal features or minor disturbances, and also potentially interacting with other objects in its vicinity. This could be evidence of a past or ongoing merger event.
