The galaxy presents a somewhat elliptical morphology, exhibiting a relatively smooth overall appearance. The color profile indicates a dominant population of older stars, leaning towards redder wavelengths in the central region and a very slight shift to bluer tones on the outskirts. While there are no prominent spiral arm structures or distinct dust lanes immediately visible, there appears to be some slight asymmetry. I would describe the galaxy as a smooth and rounded galaxy. Some disturbances may be present in the galaxy. The galaxy could also possibly be merging with another object.
