The galaxy presents as a slightly elongated, elliptical structure, lacking prominent spiral arms or a distinct disk. The light distribution appears relatively smooth and centralized, with a gradual decrease in brightness from the core outwards. There's a noticeable yellowish hue to the core, suggesting an older stellar population. Faint, indistinct bluer regions are sparsely scattered within the galaxy's diffuse outer halo, potentially indicating regions of recent, low-level star formation. There are no signs of significant tidal disturbances, mergers, or strong interactions with other galaxies. Overall, the galaxy exhibits characteristics consistent with a relatively quiescent, evolved system.
