The galaxy appears as a moderately luminous, relatively compact object. Its morphology is predominantly smooth, with a centrally concentrated light distribution suggesting an elliptical or lenticular classification. There is a possible faint, diffuse disk extending beyond the central region, but this is not well-defined. No prominent spiral arms or dust lanes are discernible in this image. The color is generally consistent with an older stellar population, showing a redder hue. There is no apparent strong evidence of ongoing major mergers or significant tidal distortions, although a very minor disturbance cannot be ruled out. The overall appearance suggests a galaxy with a significant mass and relatively low star formation activity.
