This galaxy appears to exhibit a somewhat amorphous morphology. A bright, roughly circular central region is visible. Surrounding this core is a fainter, extended halo with irregular boundaries. There are possible signs of tidal disturbance or interaction, characterized by faint plumes or extensions emanating from the main body of the galaxy. Overall, the galaxy appears to be relatively compact in size, lacking a well-defined disk structure. A significant portion of the light appears concentrated in the central region, potentially indicating an active galactic nucleus or a dense stellar population.
