The observed galaxy presents as a relatively small, somewhat elongated object. It is possible this galaxy is either elliptical or a spiral system viewed edge-on. A small degree of asymmetry is noticeable, particularly in the upper half. An area of reddish light is visible. This may be evidence of a minor disturbance or potential recent merger. The galaxy appears to be undergoing a period of relative quiescence, with no major ongoing mergers detected.