The galaxy presents a predominantly smooth morphology, exhibiting a somewhat elongated, cigar-like shape. The central region shows a higher concentration of light, appearing more luminous and yellow-orange in color, suggesting an older stellar population. Progressing outwards from the core, the galaxy displays a subtle color gradient, transitioning towards a slightly bluer hue at the edges of the disk. This implies the presence of some younger, bluer stars in the outer regions, indicative of ongoing star formation. There is no evidence of a prominent disk structure or spiral arms. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions, though there might be minor disturbances present.
