The galaxy presents a lenticular morphology, with a dominant, relatively smooth bulge and a faint, diffuse disk. The overall color profile suggests an older stellar population, with a yellowish hue throughout the bulge and a slightly bluer tint in the disk. There is evidence of some minor disturbances or asymmetry, which may suggest past interactions or minor merging events. Star formation appears suppressed. The galaxy appears to be relatively isolated, showing no clear signs of major merging or tidal interactions. It displays a moderately round shape.
