The galaxy presents a somewhat amorphous, diffuse morphology with a central concentration of light that fades outwards. It appears relatively smooth in structure, lacking distinct spiral arms or a prominent bulge. The color gradient suggests a predominantly older stellar population, with a possible hint of ongoing, but limited, star formation activity, potentially contributing to the bluer hue in the central region. The overall shape seems to be somewhere between elliptical and disk-like, but without clear distinguishing features to classify it definitively. There is a very slight indication of minor disturbance in the light distribution, hinting at a potential past interaction or minor merger event. The lack of strong color variation implies a relatively homogenous distribution of stellar populations within the galaxy. The size appears compact, suggesting a smaller dwarf galaxy or a more distant, larger system with limited spatial resolution.
