This galaxy appears to be a relatively smooth, disk-dominated spiral or lenticular galaxy viewed at a slight angle, though not quite edge-on. There is a bright central bulge that is roughly circular. The disk surrounding the bulge displays some subtle variations in color, potentially indicating some spiral arm structure, but these features are not particularly well-defined. The overall color of the galaxy suggests an older stellar population, with a greater proportion of redder stars. There is no strong evidence of active star formation present in the image. Faint, diffuse light extends beyond the main body of the galaxy, suggesting a halo of older stars. The morphology does not show any obvious signs of recent major mergers or strong tidal interactions.
