The galaxy presents as a relatively smooth, elliptical structure with a concentrated, bright central bulge. There is a subtle color gradient, with the core exhibiting a yellowish-white hue, potentially indicative of an older stellar population. The outer regions of the galaxy appear somewhat bluer in color than the core, which hints at the presence of a younger stellar population or ongoing star formation. The galaxy's overall shape is elongated, appearing closer to an in-between roundness classification. There are no prominent dust lanes or spiral arm structures visible, nor any obvious signs of tidal disturbances or major mergers. Overall, this galaxy appears to be a massive elliptical galaxy that is not particularly actively forming stars.
