This galaxy exhibits a generally smooth morphology with a concentrated central bulge. The light distribution appears relatively uniform, lacking significant spiral arm structures or prominent dust lanes. There is a slight elongation to its shape, hinting at a possible elliptical form, though it appears fairly close to round. The galaxy's color profile suggests a population of older stars, indicated by the reddish-yellow hue, which might imply a lower current star formation rate. There are no obvious signs of tidal disturbances or ongoing mergers, suggesting it is likely a relatively undisturbed system. 
