The observed galaxy appears to be a spiral galaxy exhibiting notable disk features. Definite spiral arm structures are visible, though the resolution prevents precise tracing. The galaxy presents a central bulge of moderate size and a bar-like structure that shows mild prominence. The overall color of the galaxy leans towards blue, which is indicative of active star formation. The galaxy does not seem to be perfectly isolated; there is a nearby object that could be a companion galaxy. No signs of significant tidal disruption or ongoing major merger events are immediately apparent, although minor disturbances cannot be ruled out from this image alone. The galaxy is likely a moderate-mass system with a reasonable rate of ongoing star formation, which is consistent with its relatively blue color. The apparent size suggests a reasonably large galaxy based on comparison with other objects in the field.
