The galaxy presents a relatively smooth morphology, indicating a lack of significant recent merger events. The dominant feature is a prominent, elongated disk structure, viewed nearly edge-on. The central bulge appears substantial, with a fairly smooth texture. The lack of distinct spiral arm structures suggests a classification towards the lenticular end of the Hubble sequence. The outer edges of the disk fade gradually into the background sky, lacking sharp boundaries. Color gradients are observed, with a slightly redder hue toward the central bulge and a bluer tint along the disk, possibly indicating younger stellar populations. The disk appears slightly warped or tilted, and is not perfectly flat. 
