The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution suggests a spheroid-dominated morphology, with minimal evidence of spiral arms or a well-defined disk. The galaxy appears largely featureless, exhibiting a gradual radial decline in surface brightness. The color is consistent with an older stellar population. While there are no obvious signs of a major merger, there is a hint of a minor disturbance. There appears to be ongoing, but not prolific, star formation. The galaxy appears to be an elliptical type, and it is fairly massive for its size. 