The galaxy presents an elliptical morphology. The light distribution appears smooth and concentrated, with a high degree of central luminosity. The color profile exhibits a notable red shift towards the central regions, indicating an older stellar population. Subtle blue tinges are present on the outer edges, implying a very low level of on-going star formation within the galactic disk. The overall shape tends towards an elongated form, showing the presence of a bulge component, and indicating that the galaxy is likely a disk galaxy viewed at an inclined angle. There is no strong evidence of tidal features, major mergers, or significant disturbances in its structure. The galaxy's structure is largely undisturbed.
