This galaxy exhibits a disk-like morphology with a defined central bulge and surrounding disk structure. The bulge appears relatively smooth, with a concentrated light profile. The disk shows evidence of some irregularities, possibly indicating tidal interactions or internal disturbances. The galaxy displays a color gradient, with the central regions appearing redder, potentially indicating an older stellar population, while the outer regions are bluer, suggesting ongoing star formation. Evident is a slight asymmetry, possibly due to a minor merger event. There appear to be regions of dust obscuration within the disk, and a faint tidal tail is possibly extending outwards, alluding to ongoing gravitational interactions. The spiral arms of the galaxy are not clearly defined, but there are hints of their presence in the distribution of the bluer, star-forming regions. The overall impression is of a galaxy undergoing some form of dynamical evolution.
