The galaxy presents as a spiral system, exhibiting a clear disk structure oriented at a moderate inclination to our line of sight. The central bulge appears prominent and concentrated, with a color gradient suggesting an older stellar population. Faint spiral arms emanate from the core, with varying degrees of tightness; roughly two arms are seen. Some asymmetry in the arm structure hints at possible interactions or internal disturbances. The bluer light in the outer disk possibly signifies ongoing star formation, while redder regions point to older stellar populations. Dust lanes are not readily discernible. The galaxy appears to be relatively isolated. Overall, it appears as a fairly well-defined, relatively undisturbed spiral galaxy.
