This galaxy presents as a relatively well-defined, elongated disk structure. The central region is characterized by a bright, concentrated bulge, exhibiting a yellowish hue. Fainter spiral arms are visible extending outwards from the central bulge. The arms appear somewhat tightly wound, suggesting a possible intermediate spiral galaxy type.

The overall color profile indicates a mixture of stellar populations. The central bulge leans towards older, redder stars, while the disk component shows bluer hues which may reflect the existence of younger, hotter stars and ongoing star formation. The galaxy does not present any obvious signs of major mergers or significant tidal disturbances. There may be a minor disturbance within the arms, but no major asymmetries are apparent. The general morphology is fairly smooth.
