The galaxy presents as a diffuse, elongated structure. Its overall color profile suggests a relatively old stellar population, displaying a yellowish hue. There are subtle variations in surface brightness, with a brighter, more concentrated central region that gradually fades towards the edges, giving the impression of an elliptical or lenticular morphology. The smoothness of the light distribution indicates a well-mixed stellar population, with no prominent spiral arms or distinct features easily discernible at this resolution. There's a subtle asymmetry in the overall shape and light distribution, possibly indicative of a past or ongoing interaction. The galaxy appears largely undisturbed, yet hints of a minor disturbance can be seen at the very bottom.
