The galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on. A prominent central bulge is visible, appearing relatively smooth and spheroidal with a color gradient suggesting an older stellar population concentrated towards the center. The disk component appears thin and elongated, with a faint bluish color evident along the outer edges, potentially indicating ongoing star formation. The dust lane appears patchy, with some areas of higher obscuration than others. There is no indication of strong tidal features or signs of a major merger event, but there is a hint of minor disturbances. The overall morphology is consistent with a spiral galaxy, possibly of late type, but the near edge-on view obscures any spiral arm structure.
