The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentration of light towards the center. There appears to be a gradual fading of intensity from the core outwards, lacking distinct spiral arm features. The object is not perfectly spherical. There is a potential indication of slight asymmetry or minor disturbance in its outer regions. The galaxy's color distribution suggests an older stellar population, evidenced by the yellowish to reddish hue concentrated near the core. Fainter blueish regions are present in the outer parts of the galaxy.
