This galaxy exhibits a predominantly smooth morphology, suggesting an elliptical or lenticular classification. The object displays a centrally concentrated light profile. The overall shape appears to be of intermediate ellipticity. There is no strong indication of significant spiral arm structures. A mild tidal disturbance is possible, with a faint asymmetrical extension to the upper right quadrant. The galaxy's color profile suggests a composition dominated by older stellar populations, particularly toward the galactic core. The object shows a possible color gradient, becoming slightly bluer further away from the central region. Signs of recent merger events are minimal, but a minor interaction with a smaller companion cannot be completely ruled out.
