The galaxy presents as a luminous, elongated disk, oriented nearly edge-on from our line of sight. The central bulge exhibits a concentrated, bright, yellowish-white hue, indicative of an older stellar population. Extending outwards from the bulge, the disk appears thinner and less luminous, with a subtle gradient in color. The outer edges display a bluer tinge compared to the central region, suggestive of ongoing star formation. The overall structure implies a relatively undisturbed morphology, with no immediately apparent signs of major mergers or tidal disruptions. There may be minor irregularities or faint disturbances present in the outer disk, although these are not particularly prominent. Dust lanes appear to be either minimal or obscured by the viewing angle and/or resolution.
