The galaxy presents a largely smooth and rounded morphology. The light is concentrated towards the center, with a gradual decrease in brightness outwards. There is a slight elongation, but it appears mostly circular. The color profile suggests an older stellar population, with a yellow to reddish hue in the central regions. Faint hints of bluer color are observed in the outer edges, which could indicate regions of more recent star formation, although limited. The overall appearance does not suggest any ongoing major merging events, but there may be some signs of minor disturbances present. The galaxy appears to be a relatively isolated system.
