The galaxy presents as a singular, relatively compact object. Its morphology appears largely smooth, without prominent spiral arms or a distinct disk structure. The central region exhibits a higher concentration of luminosity, possibly indicating the presence of a galactic bulge. The overall shape is generally round with no obvious asymmetry or signs of ongoing major mergers, although the possibility of minor disturbances cannot be completely excluded. The color gradient suggests a predominantly older stellar population with less ongoing star formation, and the red hue might be caused by a significant amount of dust obscuration. Based on its estimated size, this galaxy could be considered a moderately sized elliptical or lenticular galaxy.
