The galaxy presents as a relatively smooth, elongated structure with a distinct major axis. Color gradients are subtle, but present. The central region appears more concentrated, exhibiting a slightly redder hue, possibly indicating a higher density of older stellar populations. Proceeding outward from the center, there is a shift toward bluer tones along the galaxy's edges. The disk appears to be quite inclined relative to our line of sight, as judged from the elongated shape. There is little evidence of strong spiral arm structure or major disturbances. The galaxy appears relatively isolated, showing no clear signs of ongoing major mergers, but some minor irregularities in the disk's structure could indicate minor tidal interactions or internal processes. Star formation appears to be ongoing, but perhaps not at a particularly intense rate, as indicated by the moderate blueness of the outer regions and the smoothness of the morphology.
