The galaxy exhibits a spiral morphology, viewed at a slight angle, but not quite edge-on. A bright, moderately sized bulge dominates the central region, transitioning smoothly into a visible disk. Distinct spiral arms emanate from the central bulge and extend outwards, displaying a two-armed structure. These arms appear well-defined and exhibit a medium winding. The spiral arms display a relatively smooth distribution of light, without obvious clumpy star-forming regions. The overall color of the galaxy suggests a mix of stellar populations, with the bulge appearing yellower and the arms showing slightly bluer hues. The galaxy does not exhibit any obvious signs of ongoing major mergers or significant tidal disturbances. No strong bar structure is readily apparent, although a hint of a weaker bar may be present. The galaxy presents a relatively regular structure, appearing undisturbed.
