The galaxy appears to be a spiral galaxy seen edge-on. There is a distinct central bulge with a somewhat homogenous distribution of light suggesting an older stellar population. This bulge is surrounded by a faint, elongated disk. The disk appears relatively smooth, with limited indication of significant spiral arm structure or prominent dust lanes based on color. The color gradient suggests ongoing star formation, although this may be limited. The galaxy does not show signs of any major disturbances or mergers based on visual inspection. The outer edges of the disk appear somewhat diffuse and the galaxy seems mostly uniform.
