The galaxy presents a roughly elliptical morphology with a bright, concentrated central bulge. The overall color suggests a spectral energy distribution peaking in the redder wavelengths. The outer regions of the galaxy exhibit a bluer hue, suggestive of ongoing, albeit potentially low, star formation. Visual analysis indicates a possible minor disturbance, or interaction event, given the subtle asymmetry in the outer isophotes. There are no apparent spiral arm structures or dust lanes visible in the image, suggesting the galaxy is a relatively smooth system.
