The galaxy presents an overall smooth and rounded morphology, with a noticeable central bulge that appears to be a dominant feature. The bulge exhibits a yellowish hue, possibly indicating an older stellar population. Surrounding the central bulge is a faint, somewhat flattened disk structure. There's a very slight hint of spiral structure within the disk but the spiral arms are not well defined. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The overall color gradient suggests a transition from older stars in the bulge to potentially younger stars in the disk.
