The galaxy presents as a generally smooth object with a flattened, elliptical morphology. There is a central concentration of light that gradually decreases with radial distance. The color profile appears reddish-yellow, indicative of an older stellar population. Hints of a possible disk structure are present, but it is not strongly defined. There is no clear evidence of active star formation regions or significant dust lanes. Based on the galaxy's morphology and color, it could be classified as an early-type spiral galaxy. There may be minor disturbances in the structure. There is no evidence of interaction with other galaxies.
