The galaxy presents as a central, luminous bulge, surrounded by a fainter, more diffuse disk. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. The disk appears less structured, lacking prominent spiral arms or distinct dust lanes. There's a subtle color gradient across the disk, transitioning to a slightly bluer tint further from the core, possibly indicative of younger stars. The galaxy appears to be moderately massive. There are no visible signs of a major ongoing merger.
