The galaxy presents as an elliptical morphology, exhibiting a generally smooth profile with minimal apparent features. The object appears somewhat concentrated towards the center, showing a moderate ellipticity. It has an apparent size of a few arcseconds. Its color suggests an older stellar population with less recent star formation. Possible dust lanes or minor disturbances could be present, but the limited resolution makes a confident assessment difficult. There are no obvious signs of ongoing major merger activity. The galaxy looks as though it could potentially be interacting with the galaxy to its right, but that cannot be said for sure.
