The galaxy appears to be a relatively bright, early-type spiral, or possibly lenticular, galaxy seen at an oblique angle. It exhibits a smooth, centrally concentrated light distribution with a dominant bulge component. The bulge appears yellowish, indicating an older stellar population. The disk surrounding the bulge is less prominent, but still present. It seems relatively featureless, lacking well-defined spiral arms. There might be some hint of faint, diffuse blueish regions within the disk, potentially signifying areas of recent star formation, though they are not particularly active. Overall, the galaxy appears somewhat elongated, but not excessively so. There seems to be no evidence of major mergers or significant tidal disturbances in its morphology.
