The galaxy presents as a spiral type, viewed at an oblique angle relative to our line of sight. This perspective allows for a partial view of the disk structure. Evident spiral arms emanate from the central bulge, although they are not sharply defined, appearing somewhat diffuse. The color gradient suggests active star formation within the disk, with bluer hues likely indicating younger stellar populations in the spiral arms. The central bulge appears more yellow-red, possibly indicative of an older, more evolved stellar population. The overall morphology does not suggest any significant mergers or major disturbances, although some asymmetry in the outer regions of the disk might indicate minor tidal interactions in the past. The galaxy's light is moderately concentrated, with no clear evidence of a strong central bar structure. The disk appears to be quite substantial relative to the bulge, with a moderate to small bulge size.
