The galaxy presents as a smooth, rounded structure with a concentrated central bulge. A faint, extended disk is observed, contributing to its overall apparent size. There is a slight asymmetry in the outer regions, suggesting a minor disturbance or interaction. Color gradients suggest a mix of stellar populations, with bluer hues indicating younger stars potentially forming in the disk, and redder tones in the bulge indicating older stellar populations. No prominent spiral arm structure or significant dust lanes are discernible within the resolution of the image. The estimated mass range of the galaxy falls within the realm of a typical spiral, though closer to the lower end, and is actively forming stars at a moderately low rate. A small probability of a merger event can't be excluded. 
