The galaxy presents as a fairly smooth object, elliptical in shape. The central bulge is prominent, exhibiting a bright, concentrated luminosity, suggesting an older stellar population. There is a notable extension of light emanating in a slightly more vertical direction from the brighter bulge. This area is far less concentrated, suggesting a region of lower stellar density or a possible tidal interaction. The overall color profile appears slightly redder, particularly within the bulge, consistent with a galaxy that has a lower rate of ongoing star formation. There is some irregular structure and asymmetry.
