The galaxy appears as a slightly elongated, diffuse object, exhibiting a smooth light distribution. The central region is brighter, fading towards the edges. The galaxy displays a predominantly white hue with subtle hints of yellow, suggesting the presence of both young and older stellar populations. The galaxy lacks any distinct spiral arms or a well-defined nucleus, suggesting that it could possibly be an elliptical or lenticular galaxy. The overall morphology suggests a relatively evolved system with a moderately high mass. There is a potential indication of ongoing star formation within the galaxy, but it appears to be occurring at a modest rate.
