The galaxy presents as a distorted, elongated structure, suggestive of an edge-on spiral or lenticular galaxy. The central region exhibits a concentration of light with a yellowish hue, possibly indicating an older stellar population within a bulge. Extending outwards from this central region, a fainter, bluish light is observed, tracing what may be spiral arms. One end of the galaxy appears truncated or more disturbed than the other, possibly from tidal interactions. There appears to be star formation, especially toward the disturbed end of the galaxy. The overall shape deviates significantly from a perfect elliptical form, indicating some level of dynamical disturbance.
