This galaxy presents as an edge-on spiral, notable for its prominent, flattened disk morphology. The central bulge is highly pronounced, appearing as a concentrated region of intense luminosity. The bulge exhibits a smooth, rounded appearance, suggesting an evolved stellar population. The disk is relatively smooth and appears featureless, lacking any distinct spiral arm structures or prominent dust lanes, though that may be due to the resolution of the image. There is no evidence of ongoing major mergers or significant tidal disturbances. The galaxy's overall color suggests the presence of both older stellar populations within the bulge and possibly some younger, star-forming regions within the disk, although this star formation appears to be minimal. The galaxy's morphology suggests it has undergone a period of relative quiescence.
