The galaxy presents as a relatively small, elongated, and somewhat disturbed system. It has a smooth appearance with a slight hint of a disk-like structure, but it is not clearly defined. The color suggests an older stellar population, with minimal evidence of active star formation. The galaxy's shape indicates a possible transition between an elliptical and a spiral morphology, with some asymmetry that might be the result of a minor interaction or past disturbance. There is no distinct central bulge or prominent spiral arms visible. The system appears to be relatively isolated.
