The galaxy presents a lenticular morphology. It appears elongated, with a smooth, featureless central bulge dominating the structure. The disk is oriented edge-on, displaying a subtle color gradient from the core outwards. The central region exhibits a yellowish hue, suggesting an older stellar population with minimal ongoing star formation. Moving outwards from the center, the disk displays a transition to bluer tones, indicative of younger, hotter stars. There is little to no evidence of prominent spiral arms or dust lanes, consistent with a galaxy that has largely ceased active star formation. The overall structure appears undisturbed, with no obvious signs of tidal interactions or recent merger events.
