The galaxy presents a somewhat elliptical morphology. The central bulge appears bright and concentrated with a yellowish hue, suggesting a population of older stars. Moving outwards, the galactic disk exhibits a bluer coloration and is less defined, implying ongoing, though perhaps moderate, star formation. There appears to be some faint structure in the outer regions of the disk, though without higher resolution, distinct spiral arms are not readily apparent. The galaxy is moderately inclined with respect to our line of sight. There is no obvious evidence of a major ongoing merger or significant tidal disturbance, although a minor irregularity or slight asymmetry in the disk shape cannot be ruled out.
