The galaxy appears to be an elliptical galaxy, likely a lenticular or cigar shaped elliptical given its elongated morphology. It has a smooth, diffuse light distribution with no obvious spiral arm structures or dust lanes visible. The central bulge is bright and concentrated, appearing nearly white with a hint of yellow. The outer regions fade gradually into the background sky, suggesting a lack of active star formation. There are no signs of a major ongoing merger, though the slightly irregular shape indicates the possibility of a past minor interaction or merger. The galaxy's color suggests a relatively old stellar population with a low star formation rate. Overall, the galaxy appears relatively undisturbed, with a high degree of central concentration.