The galaxy presents as a relatively smooth, disk-shaped structure, viewed nearly edge-on. There is a central bulge region that appears moderately bright and somewhat extended. The disk component shows faint evidence of spiral arm structure, although it is largely diffuse and indistinct. The color profile suggests ongoing star formation, particularly within the disk where bluer hues are observed. The morphology does not exhibit strong disturbances indicative of recent major merger activity. The light distribution implies a relatively high degree of rotational symmetry.
