The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated morphology. It has a bright, yellowish core, which likely indicates an older stellar population. The galaxy is nearly round in appearance, with no obvious disk-like structure or spiral arms visible. There is no evidence of any major mergers or significant tidal disturbances affecting its structure. Based on the colors, it appears that this galaxy is not actively forming stars at a high rate. The outer regions of the galaxy fade gently into the background, suggesting a gradual decrease in stellar density.
