The galaxy presents as a disk galaxy, viewed at an oblique angle. It has a bright, prominent central bulge, likely composed of older stellar populations, exhibiting a yellowish-orange hue. The disk component, extending outwards from the bulge, appears elongated and somewhat irregular. There may be slight distortions present. Overall, there are hints of spiral arm structure, but it is faint and indistinct. The galaxy's overall color is consistent with a population of stars with relatively low rates of ongoing star formation. The shape suggests the galaxy is not perfectly circular, leaning more towards an elongated or cigar-like shape. The galaxy does not appear to be undergoing a major merger, but there may be some minor disturbances visible.
