The galaxy presents as an elongated, spindle-shaped structure, likely a highly inclined spiral or lenticular galaxy. The central region exhibits a noticeable concentration of light, appearing yellowish-red. The outer regions show fainter, bluer hues. The galaxy appears relatively smooth with no distinct spiral arm features visible in this image. The overall morphology suggests an evolved stellar population, with ongoing star formation. There is no clear evidence of tidal disturbances or interactions with other galaxies, indicating that the galaxy is relatively isolated.
