The galaxy presents a largely elliptical morphology, displaying a smooth, concentrated light profile. The central region exhibits a yellow hue, suggesting a population of older stars. No prominent spiral arm structures or dust lanes are discernible. The outer regions of the galaxy gradually fade into the background, indicating a lack of significant ongoing star formation in the outer disk, if one exists. The overall appearance suggests a relatively evolved system. There may be a faint tidal tail to the south of the object.
