This galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. Its color profile suggests it is composed of an older stellar population, as indicated by the reddish-yellow hue of its core. Some bluer regions are present, showing indications of possible star formation. The galaxy exhibits a moderate level of roundness, showing it is not highly elliptical or cigar-shaped. There is no apparent indication of any major disturbances in the image, suggesting that it is not currently undergoing a major merger.
