The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. There appears to be little evidence of a distinct disk or spiral arms. The color gradient indicates a possible shift from bluer hues in the outer regions to yellower/whiter tones towards the center, hinting at varying stellar populations, with older, redder stars dominating the central regions and younger, bluer stars potentially present in the outer parts. A small, reddish area is visible to the right of the main body, potentially indicating a region of active star formation or a tidal disturbance, however the image resolution makes a solid conclusion difficult.
