The galaxy presents as a spiral type, viewed at an angle between face-on and inclined. There is a discernible central bulge, exhibiting a moderate size relative to the overall galactic disk. Faint spiral arms extend outwards from the central region, showing a somewhat patchy distribution of light. The galaxy's structure indicates the presence of some weak to strong bar.

The color profile suggests a mix of stellar populations. The central bulge displays a yellowish hue, consistent with older, redder stars. The outer disk and spiral arms exhibit a bluer tint, indicative of younger, hotter stars and active star formation regions. There appears to be no major, dramatic signs of interactions or recent merging events, although there are minor disturbances.
