The galaxy appears to be an elliptical galaxy, exhibiting a largely smooth and featureless morphology. It possesses a centrally concentrated luminosity profile, with a relatively round shape. The galaxy's color gradient suggests an older stellar population, with a noticeable concentration of redder light in the core and a slight shift towards bluer hues in the outer regions. There is no obvious evidence of spiral arms or a prominent disk structure. There also appears to be no major disturbances present in the galaxy such as signs of on-going mergers or tidal tails, although there may be a slight disturbance in the galaxy shape. 
