This galaxy presents a somewhat indistinct morphology, appearing largely as a diffuse, centrally concentrated object. The core exhibits a yellowish-white hue, suggesting a population of older stars. The surrounding disk, though faint, displays hints of bluer regions, potentially indicating areas of more recent star formation. There are subtle irregularities in the outer edges of the disk. While a generally smooth appearance dominates, there may be minor disturbances present within the structure, but further investigation would be required to confirm. The overall impression is of a galaxy transitioning between a spiral or irregular form towards a more elliptical one, with on going star formation at a moderate rate.
