The galaxy presents a somewhat diffuse morphology, appearing as an intermediate system. There is some structure suggestive of a disk, but it is not well-defined. The central bulge appears prominent and relatively smooth. Faint tidal features or disturbances can be seen, which may indicate a recent or ongoing merger event with another smaller galaxy. The spiral arms, if present, are not tightly wound, and the overall structure looks less ordered. The color distribution suggests a mix of stellar populations, with bluer regions possibly indicating areas of recent star formation, and redder regions, particularly in the bulge, possibly dominated by older, redder stars. There is no clear dust lane visible. The galaxy is not perfectly symmetrical, and exhibits some irregularity in its outer regions.
