The galaxy appears to be an elliptical-like structure with a smooth, diffuse light profile. The central region is the brightest, exhibiting a yellow-white hue suggestive of an older stellar population. The outer regions fade gradually, showing hints of blue, potentially indicating areas of younger stars. There is a slight elongation in its overall shape, but it lacks any distinct spiral arms or a well-defined disk. It exhibits a smooth, homogenous appearance, indicative of a galaxy without significant ongoing star formation. There appear to be possible signs of a slight tidal disturbance that can be seen as a very faint plume extending outwards from the center.
