The galaxy presents as a relatively smooth, centrally concentrated object. Its light profile is generally round, with a slight elongation or intermediate shape visible in the isophotes. The core region exhibits a yellowish hue, suggesting an older stellar population and potentially a larger concentration of evolved stars. A faint disk-like structure or featured component is suggested by the slight deviation from perfect roundness, but there is no distinct arm structure that can be observed. No significant tidal disturbances or signs of recent merger activity are readily apparent in the morphology. There appears to be an absence of strong blue color, which could suggest a lower rate of on-going star formation or obscuration by dust. Overall, the galaxy appears to be a well-formed system without significant ongoing interactions.
