The galaxy appears to be relatively compact, spanning approximately 2 kpc in diameter. Its overall color suggests a mixed stellar population. The central region exhibits a more reddish hue, indicative of older, cooler stars or perhaps significant dust obscuration. The outer regions show bluer tints, which may point to ongoing or recent star formation activity.

Morphologically, the galaxy shows some signs of tidal disturbances, with an uneven distribution of light and possible asymmetries in the outer regions. A significant fraction of citizens indicate merging activity. Though blurred by the resolution of the image, there seems to be more than one nucleus of light. It does not have the classical spiral arm structure. Its light is diffuse, suggesting it may be in the process of merging with one or more satellite galaxies.
