The galaxy appears as a relatively compact object with a noticeably brighter, concentrated central region that fades into the outer edges. The overall shape is slightly elliptical, not perfectly spherical. The color profile suggests an older stellar population, showing a redder hue, particularly in the central bulge, with hints of bluer colors toward the disk or outer regions, which suggest recent star formation activity. There might be a small central bar structure. There appears to be some minor disturbance in the outer regions of the galaxy. No obvious spiral arms are visible.
