The galaxy presents as a relatively smooth, elongated structure, likely a disk galaxy seen at an angle. The central bulge is a pronounced yellowish-orange, suggesting an older stellar population. The disk component appears less defined, showing a subtle gradient in color from yellowish-orange near the bulge, fading to a greenish tint towards the outer edges, perhaps indicating some low level of ongoing star formation. There is no strong evidence of spiral arms in the image. The galaxy appears isolated, showing no clear signs of major tidal disturbances or interactions with other galaxies. The overall morphology suggests a galaxy that is likely evolving relatively peacefully, with a dominant old stellar population and possibly low levels of star formation.
