The galaxy presents as an elongated, disk-shaped structure, viewed at a high inclination. The central bulge appears relatively prominent and concentrated, exhibiting a smooth, yellowish-white hue. The outer regions of the disk show a subtle fading in brightness as radial distance increases. There's a slight asymmetry in the disk, perhaps indicating a minor interaction or disturbance event. The overall morphology suggests a late-type spiral or lenticular galaxy with little in the way of prominent spiral arm structures visible. The color is suggestive of an older stellar population, with reduced on-going star formation. No distinct dust lanes are discernible, even at this inclination.
