The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution is fairly even, with a gradual decrease in intensity moving outwards from the center.  It exhibits a yellowish-orange hue, suggesting an older stellar population with fewer young, hot stars. There is very little evidence of spiral arms or significant dust lanes within the visible structure. The overall form is quite rounded, displaying little elongation or asymmetry. A small, faint, reddish region is visible on the lower portion of the galaxy, possibly an area of localized star formation or a background object.  The galaxy shows no signs of major tidal disturbances or ongoing mergers in this image.
