The galaxy appears to be a spiral galaxy viewed at a high inclination, close to edge-on. A prominent disk is visible with evidence of spiral arm structure. The arms appear relatively tightly wound. There is a bright, moderately sized central bulge region exhibiting a yellowish hue. Fainter blue light is observed in the surrounding disk, likely indicating regions of star formation. There may be a slight bar structure present. No significant tidal disturbances or signs of a major merger are apparent, though a faint, subtle asymmetry in the disk could indicate a minor interaction. Overall, the galaxy appears to be a relatively undisturbed spiral galaxy, possibly of intermediate Hubble type.
