The galaxy presents as a slightly elongated, disk-like structure, observed at an oblique angle relative to our line of sight. The central bulge is prominent and appears yellowish, suggesting a population of older stars. Fainter, bluer light extends from the central bulge, indicating some presence of younger, hotter stars in the spiral arms or disk. There is a hint of possible merging or tidal disturbance, with some distortion apparent in the outer regions of the galaxy. Overall the galaxy appears relatively smooth, with limited distinctive features beyond a central bulge and broad, indistinct arms. There are no signs of a dust lane.
