The galaxy presents as a relatively smooth object, with a moderate degree of ellipticity. There is a central concentration of light that appears yellowish, suggesting an older stellar population dominating the core. The outer regions of the galaxy exhibit a bluer hue, indicative of younger, hotter stars and possible ongoing star formation. There are subtle indications of a possible disk-like structure or faint arms, though these features are not sharply defined. There are hints of a minor disturbance possibly due to a small merger event. Overall the galaxy appears to be in an intermediate stage of evolution, with a mix of older and younger stellar populations and a moderate star-formation rate.
