The galaxy presents a somewhat elongated, cigar-shaped morphology. A central bulge is clearly visible, exhibiting a yellowish-orange hue, suggesting an older stellar population. This core region displays a high degree of smoothness and concentration of light. Extending outwards from the central bulge is a fainter disk component. This disk appears relatively featureless in terms of distinct spiral arms, possibly indicating a more quiescent star formation rate. The galaxy shows no obvious signs of a major merger event or significant tidal disturbances, though subtle asymmetries cannot be ruled out without more detailed analysis. The galaxy is at a considerable distance, its red shift indicates that its light is shifted towards the red end of the spectrum due to its distance from us.