The galaxy presents as a relatively smooth, centralized object. The light is concentrated, exhibiting a bright, yellowish core that fades into a more diffuse, bluish halo. There are no clearly defined spiral arms or bars, suggesting a disk galaxy with a dominant bulge or perhaps an elliptical galaxy. The overall shape is somewhat elliptical, leaning towards a more rounded form rather than an elongated, cigar-like shape. There are no obvious signs of major mergers or significant tidal disturbances in the immediate vicinity, although there are subtle irregularities in the outer halo. The blue tint suggests the presence of some ongoing star formation, but the dominant yellowish light indicates an older stellar population and a cessation of active star formation. The galaxy's light distribution appears fairly even, with a gradual falloff from the center.
