This galaxy presents as a relatively smooth, elliptical morphology, exhibiting a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The color profile suggests a dominant population of older stars, indicated by the redder hues, with possibly a low level of ongoing star formation that would produce the observed bluer color, particularly in the more central region. There is no clear evidence of spiral arm structures or significant dust lanes. The general shape appears more akin to a flattened spheroid rather than a perfect circle. There are also no signs of any major mergers. It could possibly be undergoing a minor disturbance. 
