The galaxy presents an elliptical morphology, appearing somewhat flattened with an axial ratio of approximately 0.8. Its overall color appears bluish. The light is centrally concentrated, with brightness decreasing gradually towards the outer regions. The luminosity profile seems to follow a Sersic profile, suggesting a bulge-dominated system. There are no prominent spiral arms or a distinct disk structure visible, and there are no clear signs of recent major merger activity, though there might be a minor disturbance in the outer regions. There's evidence of low-level ongoing star formation.
