The observed galaxy appears to be a spiral galaxy, oriented roughly face-on from our perspective. A central bulge is distinctly visible, exhibiting a brighter, more concentrated luminosity profile. The disk component shows evidence of spiral arms, but with some irregularity. There appears to be a moderate bulge component present with a winding pattern. The galaxy's shape is elongated, and the disk exhibits faint, somewhat diffuse spiral arms. The overall color suggests a mix of stellar populations. There may be a weak bar component present with moderate disturbances visible.
