The galaxy presents as a disk galaxy, viewed at a nearly edge-on orientation. The central bulge is prominent and appears to be composed of older stellar populations, indicated by its yellow-orange hue. This central region transitions smoothly into a relatively thin, elongated disk. Dust lanes are not clearly visible, though subtle variations in surface brightness may indicate obscuration within the disk plane. The overall morphology suggests the galaxy is relatively undisturbed, showing no signs of major mergers or tidal interactions. The smoothness of the light distribution indicates a lack of significant recent star formation, consistent with the observed color profile. The shape of the galaxy appears to be a cigar shape. The light profile suggests a relatively evolved system.
