The galaxy appears to be a relatively compact system, with an overall smooth appearance. A bright, somewhat concentrated central bulge is visible, surrounded by a less defined disk. The bulge exhibits a yellowish-white hue, suggesting a population of older stars. The surrounding disk shows some evidence of bluer regions interspersed within it, hinting at ongoing or recent star formation, although the disk's structure is poorly defined. There is some subtle hint of possible disturbance or interaction based on a slight asymmetry in the outer regions of the disk. The system appears to be neither a perfect elliptical nor a well-defined spiral, possessing an intermediate morphology.
