The galaxy appears to be a spiral galaxy, oriented approximately face-on. It exhibits a strong central bar structure that spans a significant portion of the galactic core. The spiral arms are well-defined, with a mostly medium winding. There appear to be two primary spiral arms, though some fainter arm segments can be seen. The bulge is of moderate size, with a relatively bright central concentration. The overall appearance suggests a barred spiral galaxy with some signs of tidal disturbances, but it generally appears unperturbed, and not undergoing any major merging activity. The color distribution indicates regions of both older stellar populations (more prominent in the bulge) and ongoing star formation (notably in the spiral arms).
