The galaxy appears to be a spiral galaxy, although the arms are not very distinct. It presents with a relatively smooth morphology overall. A central bulge is clearly visible, appearing bright yellow-white in color, indicating a population of older stars. Fainter, bluer hues surround the central bulge and extend outwards, which could represent younger stellar populations and regions of ongoing star formation. There is some suggestion of a disk structure but its boundaries are somewhat indistinct. Based on the apparent lack of strong disturbances, the galaxy is likely not undergoing a major merger. Faint wisps or minor perturbations are visible, suggesting some interactions may have occurred or be occurring. The galaxy exhibits an intermediate roundness, neither perfectly spherical nor highly elongated, and it is inclined somewhat to our line of sight.
