The galaxy presents as a disk galaxy, viewed at a high inclination, nearing edge-on. There is a central bulge component that appears quite prominent and relatively bright. Dust lanes bisect the galaxy along its major axis, obscuring light from stars behind. These dust lanes appear somewhat patchy and uneven, hinting at potentially disturbed morphology. The galaxy disk is relatively smooth, exhibiting a lack of prominent spiral arm structure in this image. The overall color suggests a redder stellar population. The galaxy exhibits features that could be interpreted as minor disturbances, potentially indicative of a past or ongoing interaction.
