The galaxy presents as a face-on or slightly tilted spiral galaxy with a prominent central bulge. The bulge exhibits a yellowish-white hue, suggestive of an older stellar population. Fainter spiral arms are discernible extending outwards from the bulge, displaying a bluer tint, which likely indicates more recent star formation activity. The spiral arms are somewhat flocculent in appearance, lacking a highly defined, grand design structure. There appears to be some minor disturbances in the shape of the galaxy indicating the possibility of a past minor merger event. The galaxy appears relatively isolated, lacking any immediately obvious signs of interactions with other galaxies.
