The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a centrally concentrated bulge region that dominates its overall structure. The color of the galaxy appears to be relatively uniform, with a slight yellow or reddish hue in the central region, suggesting an older stellar population. There is minimal evidence of distinct spiral arms or significant dust lanes. The galaxy is well-defined. The light distribution is concentrated towards the center, with a gradual decrease in luminosity towards the outer regions. There may be minor disturbances or faint features suggesting interactions, but the overall morphology is quite uniform.
