The galaxy exhibits a generally smooth morphology, with a slightly elongated, ellipsoidal shape. The central region displays a concentrated, yellowish-white luminosity, suggesting the presence of an older stellar population. Moving outward from the center, the color transitions to a bluer hue in the outer regions, hinting at the presence of younger, hotter stars and possibly ongoing star formation, albeit at a relatively low rate. There may be some minor disturbances occurring within the system.
