The galaxy presents as a relatively smooth, elliptical structure. Its central region exhibits a bright, concentrated core with a diffuse glow, suggesting a significant population of stars and potentially an active galactic nucleus. There is a slight elongation to the galaxy's shape; it is slightly cigar-shaped, and it has some faint disk features. The color profile indicates a mix of stellar populations, with the inner regions having a slightly redder hue compared to the outer regions, hinting at older stellar populations or dust obscuration in the center. No prominent spiral arms or distinct dust lanes are visible. The overall appearance suggests a relatively evolved galaxy, possibly an elliptical or lenticular type, with ongoing though likely moderate star formation.
