This galaxy presents as a disk galaxy seen at an oblique angle. The central bulge is luminous and appears yellow, suggesting a population of older stars. The disk exhibits a bluer color, indicative of younger stars and ongoing star formation. The disk appears somewhat smooth with hints of spiral structure, though it is not well-defined, perhaps due to dust obscuration or the viewing angle. The outer regions of the galaxy fade gradually into the background, indicating a diffuse stellar halo. The galaxy's shape is elongated, with an apparent flattening ratio of roughly 0.7, deviating notably from spheroidal. There are subtle signs of asymmetry and a faint, disturbed feature suggesting possible interactions or minor mergers in its past.
