The galaxy presents as an elongated, cigar-shaped object with a smooth, diffuse morphology. A prominent central bulge is visible, exhibiting a yellowish-orange hue, which may indicate an older stellar population dominating this region. The outer regions of the galaxy show a bluer tint, suggesting the presence of younger, hotter stars and possibly ongoing star formation. There are no apparent spiral arm structures or significant dust lanes visible. The overall smooth appearance suggests a relatively undisturbed galaxy, with no major merger events evident.
