This galaxy exhibits a generally smooth morphology, with a somewhat elliptical shape. The central region is noticeably brighter and possesses a yellowish-white hue, suggesting a population of older stars. Faint, elongated extensions can be seen emanating from the central region. There are signs of possible gravitational interaction or recent merger activity which distorts the galaxy. These appear as disturbances or faint tidal features extending from the main body. The galaxy's overall color profile suggests moderate levels of ongoing star formation and a relatively high mass. 
