The galaxy presents as a somewhat elongated, lenticular or possibly an edge-on spiral system. It has a smooth, centralized bulge exhibiting a yellowish hue, suggesting an older stellar population. Faint blue colors emanate from the galaxy's disk. The disk component seems fairly uniform with some subtle texture suggesting the presence of spiral arms or dust lanes, though this is difficult to determine with certainty given the viewing angle. The overall morphology hints at a system undergoing some star formation, as indicated by the subtle bluer colors, though the rate appears to be relatively low based on the prominence of the older, yellow-toned bulge. There appear to be no signs of significant mergers or tidal disturbances in this image, with the galaxy's structure appearing relatively undisturbed. The light is quite concentrated, indicating high mass concentration.
