This galaxy appears to be an elliptical type, exhibiting a somewhat cigar-shaped morphology. The central region is bright, displaying a yellowish-orange hue, which suggests an older stellar population. The outskirts of the galaxy fade into the background, indicating a smooth, gradual decline in stellar density. There is a hint of possible tidal features or minor disturbances. The overall structure implies a galaxy with a dominant bulge component. Based on color, star formation activity appears to be suppressed.
