The galaxy presents as a smooth, elliptical object, exhibiting a significant central bulge that appears bright and concentrated. The galaxy's light profile shows a gradual decrease in intensity from the core outwards. There is a slight elongation in its shape. The overall color is indicative of an older stellar population, suggesting a relatively quiescent star formation rate. No prominent spiral arm structures or dust lanes are discernible. There may be a hint of some minor tidal disturbance in the outer regions, but further observation is needed to confirm. The galaxy does not appear to be actively merging with another object.
