This galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on from our vantage point. A central bulge is visible, exhibiting a yellowish hue, potentially indicating an older stellar population. The disk itself shows a bluer tint, suggesting the presence of younger, hotter stars and ongoing star formation. Dust lanes are not clearly resolved but may be present obscuring some regions of the disk, contributing to the mottled appearance. There are no obvious signs of major interaction or tidal features suggesting the galaxy has experienced a recent major merger, though minor disturbances are possible. The overall morphology is consistent with a spiral or lenticular galaxy seen at a high inclination. The estimated size indicates a moderately sized galaxy.
