This galaxy presents as an edge-on spiral, exhibiting a prominent disk seen nearly in its entirety along its equatorial plane. The central bulge is notable, appearing luminous and concentrated, with a smoothly elliptical morphology. The surrounding disk is extended and somewhat flattened, showing evidence of dust lanes, though they are not sharply defined. The overall color profile suggests a mix of stellar populations; the bulge appears slightly redder, potentially indicating an older stellar population, while the disk shows bluer hues suggestive of ongoing or recent star formation. There is little evidence of strong tidal interactions or major morphological disturbances. The galaxy appears relatively isolated and undisturbed, maintaining a well-defined and regular structure.
