The galaxy presents as a relatively well-defined spiral, viewed at an oblique angle. The central bulge appears to be a dominant feature, exhibiting a smooth, yellowish hue, indicative of an older stellar population. There is evidence of a disk component, although partially obscured by the viewing angle. Faint spiral arms emanate from the central bulge, displaying a bluer tint that could be a region of more active star formation. There also seems to be some minor disturbances, potentially from a tidal interaction.
