The galaxy presents as a somewhat elliptical structure, though approaching a disk-like morphology when accounting for its tilt relative to our line of sight. A bright central bulge is evident, displaying a yellowish hue suggesting an older stellar population. Extending outwards from the core, a fainter, bluer disk component is visible. This suggests ongoing star formation, though it appears relatively quiescent. The overall smoothness of the light distribution suggests it is fairly evolved, with a possible minor disturbance that could indicate some merging event or interaction.
