The galaxy appears to be a relatively smooth, elliptical type galaxy. It exhibits a generally round morphology with a slight elongation. There is no apparent spiral structure or strong disk component visible in the image. The galaxy's light distribution is concentrated towards the center, suggesting a significant bulge component. There are no obvious signs of ongoing major mergers or strong tidal disturbances; however, a minor asymmetry or disturbance cannot be entirely ruled out. The color is generally consistent with an older stellar population. The galaxy displays a magnitude range from blue to red. It appears as a redder color, possibly indicating a lack of recent star formation and a greater abundance of older, redder stars. Overall, the galaxy presents as a fairly typical elliptical galaxy at a moderate distance.
