The galaxy presents a distinct spiral structure. Two prominent arms extend outwards from a central bulge, exhibiting a relatively tight winding pattern. The bulge appears substantial and moderately bright, possibly indicating a significant population of older stars. A bar-like structure is apparent across the center, running through the bulge, appearing somewhat strong. The overall color profile suggests a mix of stellar populations. The central region displays a yellowish hue which is a characteristic of older stars, whereas the spiral arms show hints of bluer tones, implying more recent star formation activity. No obvious signs of a major merger event are apparent, although some minor disturbances may be present in the outer regions of the arms. The galaxy is viewed at a relatively face-on angle.
