The object is a spiral galaxy, observed edge-on. Its central bulge appears moderately bright with a slight yellowish hue, indicative of an older stellar population. Extending outward from the bulge is a relatively thin disk. The disk presents a gradient of colors, with the region closer to the bulge exhibiting a yellowish-white tone, transitioning to a fainter blue towards the outer edges. The blue hue suggests the presence of younger, hotter stars within the disk, and indicates ongoing or recent star formation. The galaxy shows no signs of major mergers or significant tidal disturbances. There is a slight indication of a boxy bulge. The galaxy is well-defined, with no signs of extreme irregularities. The galaxy is actively forming stars at a modest rate. The estimated stellar mass of the galaxy is substantial.
