The galaxy presents a largely elliptical morphology with a smooth, diffuse light distribution, suggesting an older stellar population with limited ongoing star formation. The central region exhibits a high concentration of light, appearing nearly spherical. There is no clear evidence of spiral arm structures or significant dust lanes. Slight elongation in the overall shape is observed, and a very faint disk could be present. No signs of tidal tails or major disturbances are apparent, indicating that it is likely not undergoing a major merger event. The galaxy's color appears to be shifted slightly towards the red end of the spectrum.
