The galaxy exhibits a generally smooth morphology, with a high degree of central concentration of light. The galaxy presents an elliptical or lenticular shape, appearing mostly round, although there is a slight elongation. The color gradient suggests a redder core transitioning to bluer outer regions. There is no readily discernible evidence of spiral arm structure or other prominent disk features. The galaxy is reasonably isolated, with no obvious signs of ongoing major merger events. The smooth appearance indicates that the galaxy's light is dominated by an older stellar population.
