The galaxy appears to be a relatively smooth, elongated system, likely an elliptical or lenticular type galaxy. The central bulge is bright and concentrated, exhibiting a yellowish-white hue, suggesting an older stellar population dominates the core. The outer regions of the galaxy display a faint, diffuse blue glow, possibly indicating a small amount of recent star formation within the disk. The galaxy's shape is decidedly cigar-shaped, indicating a high ellipticity and a potential lack of spiral arm structures. There is no obvious evidence of major mergers or tidal disturbances.
