The galaxy presents as a relatively smooth, elongated structure. It is likely an elliptical or lenticular galaxy viewed at an angle. The central region exhibits a higher surface brightness, indicating a concentration of stars. The color gradient suggests a population of older stars dominating the light output, with a yellow-red hue. There may be very slight evidence of a disk. There are no obvious indications of any mergers or major disturbances, though slight asymmetries cannot be ruled out.
