The galaxy appears to be an elliptical type, characterized by a smooth, centrally concentrated light distribution. It exhibits a generally round morphology, lacking any distinct spiral arms or bar-like features. The central region displays a bright, possibly active galactic nucleus (AGN), indicated by the concentrated luminosity. The galaxy's color is predominantly redder, suggesting an older stellar population with a lower rate of star formation. There is no visual evidence of ongoing major mergers or significant tidal disturbances; however, subtle irregularities in the outer regions cannot be entirely ruled out given the image resolution. The overall appearance is consistent with a massive galaxy, exhibiting a smooth and evolved structure.
