The galaxy presents an elliptical morphology, with a smooth, concentrated luminosity profile. The central region exhibits a yellowish-orange hue, suggesting an older stellar population dominated by evolved stars. Moving outward from the center, the light gradually fades, though the colour is still somewhat yellowish. The shape of the galaxy appears somewhat elongated, deviating from a perfectly spherical form, hinting at a possible classification as an E4-E6 elliptical on the Hubble sequence. No distinct spiral arms or dust lanes are apparent, and there is no indication of active star formation within the galaxy. The overall structure appears relatively undisturbed, with no signs of recent merger activity or tidal distortions.
