The galaxy presents as a generally smooth object, with a moderate ellipticity. There may be a slight hint of a disk structure, but it appears subdued. The color profile suggests a redder, more evolved stellar population, with some central concentration. There is weak indication of disturbances in the galactic structure. The overall morphology appears to lean toward an elliptical galaxy, potentially with some ongoing or recent star formation activity. The half-light radius of the galaxy suggests that it is a normal sized galaxy. The slight bluer color suggests that the star-formation rate is relatively high.
