The galaxy presents as a centrally concentrated object with a smooth appearance. Its morphology suggests a likely classification as an elliptical galaxy, potentially of type E3-E5, given its elongation. There is a slight asymmetry observed in its light distribution, indicating a possible minor interaction or internal disturbance. The overall color is subtly redder than a typical spiral galaxy. There is no distinct disk or spiral arm structure visible. The absence of significant blue light suggests relatively low ongoing star formation.
