The galaxy presents as a luminous, elongated structure with a notable central bulge. Its overall shape is reminiscent of a flattened spheroid or a thick disk seen edge-on. The core region displays a bright, concentrated glow, suggesting a high density of stars or perhaps an active galactic nucleus. The outer regions of the galaxy exhibit a more diffuse, less intensely illuminated character. There are subtle color variations within the galaxy; a yellowish hue dominates the central regions, while the outer edges show hints of bluer tones. This may indicate the presence of younger, hotter stars in the galactic outskirts, a region that suggests evidence of ongoing star formation. There is no obvious spiral arm structure visible in this imagery, nor any substantial signs of galactic mergers or tidal disturbances. Overall, the galaxy appears to be a relatively undisturbed system, though its tilted orientation limits our ability to definitively classify it.
