The galaxy presents a largely smooth morphology, with a highly circular shape and a notable lack of discernible spiral arms or a prominent bar. Its color profile suggests an older stellar population, exhibiting a yellowish-red hue that intensifies towards the galactic core, indicating a high concentration of evolved stars. While a core is easily distinguishable, there is a very faint, diffuse halo surrounding the primary luminosity. There is no strong evidence of any ongoing major merger activity or tidal disturbances affecting the galaxy's overall structure.
