The galaxy appears to be an elliptical type, exhibiting a smooth, diffuse light distribution without prominent spiral arms or a well-defined disk structure. The central region shows a concentration of older stars, indicated by the yellowish-orange hue. The outer regions of the galaxy display a bluer tint suggesting the presence of some younger stars. The overall shape is elongated, appearing cigar-shaped and with no obvious signs of tidal disturbances or interaction with neighboring galaxies. It shows a relatively low rate of star formation.
