The galaxy appears as an elongated, disk-like structure, seen nearly edge-on from our vantage point. The central bulge is prominent and exhibits a smooth, concentrated luminosity profile, indicative of an older stellar population and/or significant dust obscuration. The disk itself shows a subtle color gradient, transitioning from a yellowish hue in the inner regions near the bulge to a slightly bluer tint in the outer edges. There are no apparent spiral arm structures or significant star-forming regions visible within the disk, possibly due to the edge-on orientation or a lack of recent star formation activity. There is no sign of any major interaction or tidal features, which suggests that the galaxy has likely not undergone a major merger event recently, however a minor disturbance cannot be ruled out. The overall morphology suggests a relatively quiescent disk galaxy, potentially a lenticular type.
