The galaxy presents a largely smooth and symmetrical morphology, appearing approximately round in shape. There is little or no indication of spiral arms or a prominent disk structure. The galaxy exhibits a centrally concentrated luminosity profile, with the brightest region residing at the galactic center. The light gradually diminishes towards the outer regions of the galaxy.

The color profile displays a somewhat homogenous distribution of red, green, and blue light with a faint red hue. These colors are relatively uniform throughout the galaxy, suggesting a lack of significant color gradients or distinct stellar populations. There's no indication of significant ongoing star formation based on the homogenous colors and smooth appearance. Furthermore, there is no evidence of tidal tails, strong distortions, or other indications of ongoing or recent major merger events. The overall appearance suggests a galaxy that is relatively undisturbed and evolved, likely an elliptical or lenticular type, with a substantial stellar mass and a low star formation rate.
