The galaxy presents an elliptical morphology with a bright, concentrated central bulge. This bulge exhibits a yellowish-white color, suggesting an older stellar population. Extending outwards from the bulge is a fainter disk. This disk demonstrates a blue hue, hinting at the presence of ongoing star formation. There appear to be no distinct spiral arm structures, and the overall light distribution is relatively smooth. Some minor disturbances appear present. Overall the galaxy appears relatively massive and currently producing stars at a modest rate.
