The galaxy appears to be an elliptical type, with a smooth, spheroidal light distribution that lacks prominent spiral arms or a distinct disk structure. The central region exhibits a higher surface brightness, gradually decreasing towards the outer edges of the galaxy. The overall color is somewhat red, suggesting an older stellar population. There appears to be a slight deviation from perfect elliptical symmetry, possibly indicating a minor interaction or disturbance. No strong evidence of an active galactic nucleus or significant star formation is immediately apparent from the available imagery.
