The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated light profile, suggesting an older stellar population dominates. The core region is bright and compact, indicating a possible accumulation of stars. The outer regions of the galaxy display a more diffuse luminosity, with a faint, extended halo. There is a slight deviation from perfect sphericity, showing a hint of elongation along one axis. There are no obvious signs of spiral arm structure or significant dust lanes. There is some evidence of minor disturbance but this is not significant enough to consider it a merger. Overall, this galaxy presents a well-defined, smooth morphology characteristic of early-type galaxies.