The galaxy presents as an elongated, cigar-shaped structure. The central bulge exhibits a bright, relatively smooth, and concentrated appearance, displaying a yellowish hue, suggesting an older stellar population. Moving outwards from the core, a flattened disk component is observed. Hints of bluer regions are present, potentially indicative of ongoing star formation within the disk. The galaxy appears relatively undisturbed, lacking any obvious signs of major mergers or tidal interactions. The overall morphology indicates a potentially late-type spiral galaxy viewed at a high inclination.
