The galaxy presents a relatively smooth and featureless appearance. Its morphology is primarily elliptical, appearing somewhat spheroidal with a slight elongation. The color distribution suggests a dominant population of older stars, with the central region exhibiting a yellowish hue characteristic of evolved stellar populations. The outer regions show a slight decrease in surface brightness, gradually fading into the background. No prominent spiral arms, dust lanes, or signs of active star formation are discernible in this image. There is no obvious evidence of a major ongoing merger or significant tidal disturbances. The overall light profile is concentrated towards the center, suggesting a high degree of central mass concentration.
