The observed galaxy presents as a near edge-on disk galaxy. The galactic disk appears significantly flattened and elongated, exhibiting a clear major and minor axis. The central bulge region appears prominent, displaying a yellowish-orange hue indicative of an older stellar population. Moving outward from the bulge, the disk shows a transition to a bluer color profile, suggesting younger, hotter stars and possibly ongoing star formation within the spiral arms, though definitive arm structures are not clearly resolved in this view. The outer regions of the disk exhibit a faint, diffuse glow. The overall morphology indicates a relatively high inclination angle with respect to the observer's line of sight. There is no obvious evidence of a major ongoing merger or significant tidal distortions.
