The galaxy exhibits a largely smooth morphology, suggesting a classification towards elliptical or lenticular. There is a slight elongation of the galactic structure, deviating from a perfectly circular form. The light profile appears centrally concentrated with a gradual decrease in brightness moving outwards from the core. The color index indicates an older stellar population, with a yellow hue in the central region. This suggests a lower rate of recent star formation activity. There is no apparent evidence of a significant ongoing merger or tidal disturbance affecting its overall structure, implying a gravitationally stable system.
