The galaxy presents as a single, somewhat symmetrical object. Its morphology appears largely smooth, lacking any visually distinct spiral arms or bar structures. The central region exhibits a brighter, more concentrated luminosity, indicating a prominent bulge. The overall shape tends towards round rather than elongated, though subtle deviations are visible.

There's an indication of a color gradient within the galaxy. The central bulge appears slightly redder in comparison to the outer regions, which exhibit a bluer hue. This may imply the presence of older stellar populations in the center and comparatively younger populations in the outskirts, suggestive of ongoing star formation. There are no obvious signs of major mergers or significant tidal disturbances affecting the galaxy's overall structure.
