The galaxy presents as an edge-on spiral, with a prominent, centrally concentrated bulge. The bulge exhibits a color profile tending towards yellow-white, suggesting an older stellar population with diminished recent star formation. A disk component is visually apparent, seen edge-on, extending significantly beyond the bulge. There are no clear signs of prominent spiral arms or distinct dust lanes, though limited resolution may obscure finer details. The disk component appears relatively smooth and featureless, with a blueish hue, indicative of the presence of younger stars. Overall, the galaxy appears undisturbed with no visible evidence of an ongoing major merger. There may be minor morphological peculiarities within the disk, potentially indicative of a minor interaction or internal disturbance.
