This galaxy exhibits a generally smooth morphology, with a slight elongation. The central region displays a concentrated luminosity, suggesting a well-defined nucleus. Some features of a spiral structure are visible, most notably some diffuse arms extending from the central bulge. The disk is observed to be relatively inclined. The color profile indicates an older stellar population, with a redder hue overall, with some pockets of blueish light. The galaxy's smooth appearance suggests it may be an elliptical galaxy that may be the result of a recent merger. Patches of dust may also be present. 
