The galaxy presents as a centrally concentrated object, likely an elliptical or lenticular galaxy. It exhibits a smooth, somewhat spheroidal morphology with minimal discernible internal structure or spiral arm features. The central region is noticeably brighter and yellowish-white in color, suggesting a concentration of older stellar populations. Moving outward from the core, the color transitions to a redder hue. The galaxy appears relatively isolated, with no obvious signs of recent major mergers or tidal disturbances in this image, although some minor irregularities cannot be ruled out at this resolution. There is a lack of blue color, indicating a subdued rate of recent star formation. The galaxy is moderately bright, with no distinct isophotal twisting observed.
