The galaxy presents as a relatively smooth, elongated structure, exhibiting a noticeable disk-like morphology. The central region appears bright and concentrated, possibly indicative of a significant galactic bulge or active galactic nucleus, but more data would be needed to make such a claim. The color profile indicates the presence of both older stellar populations, contributing to a reddish hue in parts of the galaxy, and younger, star-forming regions with a somewhat blueish tone. The overall structure seems undisturbed, without significant signs of recent major merger events, although faint distortions or tidal features might exist at the outer edges but are difficult to discern from the quality of this image. The orientation of the galaxy provides a nearly edge-on view. The estimated size of the galaxy appears moderate. The low star formation rate and the morphology suggest a late-type disk galaxy or potentially an early-type disk galaxy.
