The galaxy presents as a lenticular or possibly a spiral galaxy viewed at a high inclination, nearly edge-on relative to our line of sight. It appears to be moderately sized with a significant central bulge that is slightly brighter and more condensed than the surrounding disk. The bulge appears slightly more yellow-red in color, indicating an older stellar population. The disk component shows evidence of spiral arms, albeit poorly defined, primarily noted by slight color variations rather than distinct morphological features. These color variations may indicate areas of recent or ongoing star formation. There appears to be minor disturbances in the disk’s morphology possibly indicating a past or ongoing interaction. Overall, the galaxy exhibits an intermediate stage of evolution, having likely undergone a significant amount of star formation in the past but possibly retaining some gas and dust for future stellar activity.
