The galaxy presents a predominantly smooth morphology with a high degree of central concentration. Its shape appears largely rounded, displaying minimal elongation. There is a suggestion of a faint disk-like structure or possible tidal feature extending away from the main body, although this is not sharply defined. 

The color gradient suggests that the galaxy possesses a significant population of older stars toward the center, while hints of bluer colors in the outer regions could indicate more recent star formation. Overall, there is an indication of low levels of ongoing star formation. There is no readily visible evidence of a major ongoing merger event; however, a minor interaction or disturbance is not definitively ruled out.
