This galaxy exhibits a somewhat lenticular morphology, displaying a prominent central bulge that appears relatively smooth and concentrated. The disk component shows a blue hue, suggesting the presence of younger stellar populations and ongoing star formation. There is a faint suggestion of spiral arm structure, though it is not well-defined. The galaxy appears to be relatively isolated, with no obvious signs of recent major mergers or tidal interactions, though some minor disturbances cannot be ruled out. It displays a moderate redshift, indicating it is at a considerable cosmological distance. The overall structure suggests a galaxy in transition, possibly evolving from a more active spiral towards a more quiescent lenticular state.
