The galaxy appears as an elongated structure, strongly suggesting an edge-on spiral or lenticular morphology. There is a noticeable central bulge that seems to dominate the galaxy's overall luminosity profile. It exhibits a generally rounded shape. The disk component is difficult to resolve into distinct spiral arms, appearing more as a flattened distribution of light and color. The disk's orientation is almost perfectly edge-on, contributing to this effect. The disk shows hints of obscuring dust lanes, though detailed structures are hard to distinguish at this resolution.

The galaxy's overall color suggests an older stellar population, especially towards the bulge. The disk shows a similar hue, but with a slight blue tint, potentially indicative of more recent star formation. No signs of major merger events are present and the galaxy appears mostly undisturbed.
