The galaxy exhibits a primarily smooth morphology, with a concentrated central bulge that appears roughly circular. The galaxy presents a yellow-white hue in its central region, suggesting a population of older stars. Fainter blue light is detected extending out from the central region. The outer regions are less defined and show some faint hints of potential features, but the resolution is not sufficient to definitively classify these as spiral arms or irregular structures. There is a suggestion of a minor disturbance in the overall shape and structure of the galaxy, possibly hinting towards a merging event or interaction.
